This question is a classic 'Science vs. Sci-Fi' filter. It tests if you can distinguish between electromagnetic/atmospheric effects (Solar Storms) and tectonic/mechanical effects (Tsunamis). While standard Geography books cover Auroras and Radio disruption, the specific impacts on Power Grids and Satellite Drag are often found in Science & Tech current affairs (e.g., Solar Cycle 25 or Aditya-L1 coverage).
How this question is built
This question can be broken into the following sub-statements.
Tap a statement sentence to jump into its detailed analysis.
Statement 1
Can major solar storms (solar flares or coronal mass ejections) disrupt or disable GPS and satellite navigation systems?
Origin: Direct from books
Fairness: Straightforward
Book-answerable
From standard books
Physical Geography by PMF IAS, Manjunath Thamminidi, PMF IAS (1st ed.) > Chapter 5: Earths Magnetic Field (Geomagnetic Field) > Effects of Geomagnetic Storms > p. 68
Presence: 5/5
“• The ionosphere gets heated & distorted, which means that long-range radio communication that is dependent upon sub-ionospheric reflection can be difficult.• Ionospheric expansion can increase satellite drag, and it may become difficult to control their orbits.• Geomagnetic storms disrupt satellite communication systems like GPS.• Astronauts would face high radiation levels.• Electric power grids would see a high increase in voltage that would cause blackouts.”
Why this source?
- Directly asserts that geomagnetic storms disrupt satellite communication systems such as GPS.
- Describes related effects (ionospheric heating/distortion and increased satellite drag) that can impair satellite navigation and orbit control.
Physical Geography by PMF IAS, Manjunath Thamminidi, PMF IAS (1st ed.) > Chapter 2: The Solar System > Solar Wind > p. 24
Presence: 4/5
“• The solar wind is made of plasma (ionised atoms), a stream of energised, charged particles, primarily electrons and protons, flowing outward from the Sun at speeds as high as 900 km/s and at a temperature of 1 million °C.”
Why this source?
- Defines the solar wind as a stream of energetic charged particles (electrons and protons) that drive space weather.
- Identifies the physical agent capable of disturbing Earth's magnetosphere and ionosphere, the pathways for navigation disruption.
Environment and Ecology, Majid Hussain (Access publishing 3rd ed.) > Chapter 12: Major Crops and Cropping Patterns in India > Biotic: Living > p. 122
Presence: 3/5
“Solar energy: Energy derived from the Sun. Solar wind: Clouds of ionised (charged) gases emitted by the Sun and travelling in all directions from the Sun's surface. Efects on Earth include auroras, disturbance of radio signals, and possible infuences on weather. Solifuction: Gentle down-slope movement of a saturated surface material (soil and regolith), in various climatic regimes, where temperatures are above freezing. Solum: A true soil profle in the pedon, ideally, a combination of A and B horizons. Solution: Te dissolved load of a stream. Specifc humidity: Te mass of water vapour (in grams) per unit mass of air (in kilograms) at any specifed temperature.”
Why this source?
- Notes that solar wind effects include disturbance of radio signals, which are essential to satellite navigation.
- Links solar emissions to observable impacts (auroras, signal disturbance) relevant to communications and navigation.
Statement 2
Can major solar storms (solar flares or coronal mass ejections) cause tsunamis in equatorial regions?
Origin: Weak / unclear
Fairness: Borderline / guessy
Indirect textbook clues
Physical Geography by PMF IAS, Manjunath Thamminidi, PMF IAS (1st ed.) > Chapter 15: Tsunami > 15. Tsunami > p. 191
Strength: 5/5
“because of their long wavelengths, although the attractions of the Moon and Sun play no role in their formation.
• Earthquakes (e.g. 2004 Indian Ocean Tsunami), volcanic eruptions (e.g. tsunami caused by the violent eruption of Krakatoa in 1883), landslides (tsunami caused by the collapse of a section of Anak Krakatoa in 2018), underwater explosions, meteorite impacts, etc. have the potential to generate a tsunami.• Subduction zones off Chile, Nicaragua, Mexico and Indonesia have created killer tsunamis. The Pacific among the oceans has witnessed the most number of tsunamis (over 790 since 1990).”
Why relevant
Lists the established physical causes of tsunamis (earthquakes, volcanic eruptions, landslides, underwater explosions, meteorite impacts) — i.e., events that displace large volumes of water.
How to extend
A student could use this pattern to check whether solar storms are known to produce similar sudden, large-scale water displacements (they are not listed here).
Geography of India ,Majid Husain, (McGrawHill 9th ed.) > Chapter 17: Contemporary Issues > Causes > p. 15
Strength: 5/5
“A tsunami can be generated when the plate boundaries abruptly deform and vertically displace the overlying water. Such large vertical movements of Earth's crust occur at plate boundaries. Subduction earthquakes are particularly effective in generating tsunami. Also, one tsunami in the 1940s in Hilo, Hawaii, was actually caused by an earthquake on one of the Aluetian Islands in Alaska. That earthquake measured was 7.8 on the Richter Scale. Tsunami takes place when a”
Why relevant
Explains that tsunamis are typically generated by abrupt vertical deformation of Earth's crust at plate boundaries, emphasizing mechanical displacement as the key mechanism.
How to extend
A student can compare this mechanical source requirement with the physical effects of solar storms (do they cause crustal vertical displacement?) to assess plausibility.
Physical Geography by PMF IAS, Manjunath Thamminidi, PMF IAS (1st ed.) > Chapter 5: Earths Magnetic Field (Geomagnetic Field) > Geomagnetic Storms > p. 68
Strength: 4/5
“• Solar activity drives the space weather (varying conditions in the magnetosphere). If the solar wind is weak, the magnetosphere expands, if it is strong, it compresses the magnetosphere & more of it gets in.• Periods of intense solar activity, called geomagnetic storms, occur when a coronal mass ejection erupts above the Sun & sends a shock wave through the Solar System. It takes just two days for the shock wave to reach the Earth. At the Earth's surface, a magnetic storm is seen as a rapid drop in the Earth's magnetic field strength.• Ring Current: Ring current is the name given to the large electric current that circles the Earth above its equator during magnetic storms.”
Why relevant
Describes geomagnetic storms from coronal mass ejections and notes effects on the magnetosphere and ring currents above the equator — showing where solar storms act (magnetic/space environment).
How to extend
A student could combine this with the displacement-based causes of tsunamis to evaluate whether magnetospheric disturbances have a plausible pathway to displace ocean water.
Environment and Ecology, Majid Hussain (Access publishing 3rd ed.) > Chapter 8: Natural Hazards and Disaster Management > Characteristics of Tsunami Waves > p. 33
Strength: 4/5
“Te salient characteristic features of tsunami waves are given below: • 1. Tsunamis are high energy sea waves caused mainly by the deep focus earthquakes of high magnitude.• 2. Te wavelength of tsunami waves may be more than 100 km.• 3. Te wave height of a major tsunami in the deep oceans is very low, say about a metre or so.• 4. Te speed of tsunami increases with ocean depth and vice versa. Normally the speed of a tsunami varies between 500 to 1000 kms per hour.• 5. Te wavelength of the tsunami decreases as it approaches the shallow seas and coastal areas.”
Why relevant
States that tsunamis are high-energy sea waves caused mainly by deep-focus, high-magnitude earthquakes and highlights their long wavelengths and speed dependence on ocean depth.
How to extend
A student can use these characteristic scales (energy, wavelength, speed) to judge whether effects associated with solar storms could produce comparable energy and spatial scales in the ocean.
Physical Geography by PMF IAS, Manjunath Thamminidi, PMF IAS (1st ed.) > Chapter 11: Volcanism > 11.10. Destructive Effects of Volcanoes > p. 159
Strength: 3/5
“• Showers of cinders and bombs can cause damage to life. E.g. the eruption of Mount Vesuvius in 79 AD.• Tsunamis can be generated in large water bodies due to violent eruptions. E.g. 1883 Krakatoa eruption.• The collapse of the volcanic landforms in seas and oceans causes tsunamis. E.g. 2018 Sunda Strait tsunami.• The ash from a larger eruption dispersing over a large area can lower temperatures on a regional or global scale. This could trigger famines on a large scale. E.g. 1815 eruption of Mount Tambora.• In Hawaiian-type eruption, a single flow spreads widely over open slopes or down the valleys as lava rivers engulf entire cities.• Lahars (a violent type of mudflow or debris flow) can bury entire cities in a matter of minutes causing a high number of causalities.”
Why relevant
Gives an example that volcanic collapses and violent eruptions in the ocean can generate tsunamis, reinforcing that large localized physical disturbances of water/sea floor produce tsunamis.
How to extend
A student might contrast these localized mechanical disturbances with the typically non-mechanical, electromagnetic/space effects of solar storms to assess causality.
Statement 3
Can major solar storms (solar flares or coronal mass ejections) damage power grids and electrical transformers on Earth?
Origin: Web / Current Affairs
Fairness: CA heavy
Web-answerable
"Those events also produce the most destructive space weather at Earth, with damaging consequences ranging from communication and GPS blackouts to the loss of high-orbiting satellites and power transformers on the ground."
Why this source?
- Directly states that coronal mass ejections/eruptive flares produce the most destructive space weather at Earth.
- Specifically lists loss of power transformers on the ground as a damaging consequence.
"Currents induced in ground systems can disrupt and damage power grids and pipelines."
Why this source?
- Explains that energetic particles and induced currents are hazards from space weather.
- Explicitly says currents induced in ground systems can disrupt and damage power grids and pipelines.
"CMEs can cause large geomagnetic storms that affect terrestrial systems such as electric power grids."
Why this source?
- States that CMEs can cause large geomagnetic storms when aimed at Earth.
- Links those geomagnetic storms to effects on terrestrial systems such as electric power grids.
Physical Geography by PMF IAS, Manjunath Thamminidi, PMF IAS (1st ed.) > Chapter 5: Earths Magnetic Field (Geomagnetic Field) > Geomagnetic Storms > p. 68
Strength: 5/5
“• Solar activity drives the space weather (varying conditions in the magnetosphere). If the solar wind is weak, the magnetosphere expands, if it is strong, it compresses the magnetosphere & more of it gets in.• Periods of intense solar activity, called geomagnetic storms, occur when a coronal mass ejection erupts above the Sun & sends a shock wave through the Solar System. It takes just two days for the shock wave to reach the Earth. At the Earth's surface, a magnetic storm is seen as a rapid drop in the Earth's magnetic field strength.• Ring Current: Ring current is the name given to the large electric current that circles the Earth above its equator during magnetic storms.”
Why relevant
Describes geomagnetic storms driven by coronal mass ejections and notes a 'ring current' — a large electric current that circles the Earth during magnetic storms.
How to extend
A student could extend this by noting that large space‑current systems can induce voltages in long ground-connected conductors (like power lines), potentially harming transformers and grid equipment.
Physical Geography by PMF IAS, Manjunath Thamminidi, PMF IAS (1st ed.) > Chapter 2: The Solar System > Solar Wind > p. 24
Strength: 4/5
“• The solar wind is made of plasma (ionised atoms), a stream of energised, charged particles, primarily electrons and protons, flowing outward from the Sun at speeds as high as 900 km/s and at a temperature of 1 million °C.”
Why relevant
Defines the solar wind as a stream of energized, charged particles (plasma) from the Sun with high speeds.
How to extend
Combine this with the idea that arriving charged particle streams (CME shocks) disturb Earth's magnetic environment and can drive the currents mentioned in (1) that affect infrastructure.
Environment and Ecology, Majid Hussain (Access publishing 3rd ed.) > Chapter 12: Major Crops and Cropping Patterns in India > Biotic: Living > p. 122
Strength: 4/5
“Solar energy: Energy derived from the Sun. Solar wind: Clouds of ionised (charged) gases emitted by the Sun and travelling in all directions from the Sun's surface. Efects on Earth include auroras, disturbance of radio signals, and possible infuences on weather. Solifuction: Gentle down-slope movement of a saturated surface material (soil and regolith), in various climatic regimes, where temperatures are above freezing. Solum: A true soil profle in the pedon, ideally, a combination of A and B horizons. Solution: Te dissolved load of a stream. Specifc humidity: Te mass of water vapour (in grams) per unit mass of air (in kilograms) at any specifed temperature.”
Why relevant
Lists effects of solar wind on Earth including auroras and 'disturbance of radio signals', i.e., that solar activity can disrupt human technology.
How to extend
A student could generalize that if radio systems are disturbed by solar events, other long-range electrical systems (power grids) might also be vulnerable via electromagnetic effects.
Science ,Class VIII . NCERT(Revised ed 2025) > Chapter 13: Our Home: Earth, a Unique Life Sustaining Planet > 13.3.3 Magnetic field of the Earth > p. 217
Strength: 4/5
“Other particles come from the Sun and are called the solar wind. These particles can be harmful as they can damage the atmosphere, reduce the ozone layer, and let in more harmful UV rays, which can affect life on Earth. Thankfully, the Earth's magnetic field acts like a protective shield. It pushes many of these harmful particles away from the Earth, keeping our atmosphere, and hence life on our planet safe. Earth's unique position in the solar system—allows the presence of liquid water—along with its size, atmosphere, and magnetic field, all help make it a planet where life can emerge and thrive.”
Why relevant
States solar particles can be harmful and that Earth's magnetic field acts as a protective shield against them.
How to extend
One can infer that when the magnetosphere is strongly disturbed (weakened or compressed during storms), more energetic particles/current systems reach near-Earth space and ground, increasing risk to surface infrastructure.
Physical Geography by PMF IAS, Manjunath Thamminidi, PMF IAS (1st ed.) > Chapter 5: Earths Magnetic Field (Geomagnetic Field) > A Planet's Magnetic Field Protects its Atmosphere > p. 69
Strength: 3/5
“• As the solar wind approaches a planet that has a well-developed magnetic field (such as Earth, Jupiter and Saturn), the particles are deflected by the magnetosphere, which causes the particles to travel around the planet rather than bombarding the atmosphere or surface. Whereas planets with a weak or non-existent magnetosphere are subject to atmospheric stripping by the solar wind.• Venus, the nearest and most similar planet to Earth in the Solar System, has an atmosphere 100 times denser than our own, with little or no geomagnetic field. This is a strange exception.”
Why relevant
Explains that a planet's magnetosphere deflects solar wind particles, implying that magnetic-field disturbances change how particles interact with the planet.
How to extend
A student could reason that significant magnetospheric disturbance (during CMEs) alters current flows and coupling to the ground, enabling geomagnetically induced currents in power networks.
Statement 4
Can major solar storms (solar flares or coronal mass ejections) produce intense auroras visible over much larger portions of the Earth than usual?
Origin: Direct from books
Fairness: Straightforward
Book-answerable
From standard books
Physical Geography by PMF IAS, Manjunath Thamminidi, PMF IAS (1st ed.) > Chapter 5: Earths Magnetic Field (Geomagnetic Field) > Geomagnetic Storms > p. 68
Presence: 4/5
“• Solar activity drives the space weather (varying conditions in the magnetosphere). If the solar wind is weak, the magnetosphere expands, if it is strong, it compresses the magnetosphere & more of it gets in.• Periods of intense solar activity, called geomagnetic storms, occur when a coronal mass ejection erupts above the Sun & sends a shock wave through the Solar System. It takes just two days for the shock wave to reach the Earth. At the Earth's surface, a magnetic storm is seen as a rapid drop in the Earth's magnetic field strength.• Ring Current: Ring current is the name given to the large electric current that circles the Earth above its equator during magnetic storms.”
Why this source?
- Identifies coronal mass ejections (CMEs) as the cause of geomagnetic storms and notes that strong solar wind compresses the magnetosphere so more of it 'gets in'.
- Links CMEs to rapid changes in Earth's magnetic field, a necessary condition for expanded auroral activity.
Physical Geography by PMF IAS, Manjunath Thamminidi, PMF IAS (1st ed.) > Chapter 2: The Solar System > Aurora > p. 24
Presence: 4/5
“• An aurora is a natural light display in the sky, predominantly seen in the high latitude (Arctic and Antarctic) regions (due to magnetic field lines of earth and solar wind).• Auroras are caused by charged particles, mainly electrons and protons, entering the atmosphere from above causing ionisation and excitation of atmospheric constituents, and consequent optical emissions.
Page 24”
Why this source?
- Explains that auroras are produced by charged particles (electrons and protons) entering the atmosphere along magnetic field lines.
- States auroras are normally concentrated at high latitudes, implying that any increase in incoming charged particles can modify their extent.
Physical Geography by PMF IAS, Manjunath Thamminidi, PMF IAS (1st ed.) > Chapter 5: Earths Magnetic Field (Geomagnetic Field) > Auroras > p. 66
Presence: 4/5
“• Aurora is the name given to the luminous glow in the upper atmosphere of the Earth which is produced by charged particles (solar wind) descending from the planet's magnetosphere.• Positive ions slowly drift westward, and negative ions drift eastward, giving rise to a ring current. This current reduces the magnetic field at the Earth's surface.”
Why this source?
- Describes auroras as luminous upper-atmosphere emissions caused by charged particles descending from the magnetosphere.
- Notes the ring current and associated magnetic-field reduction during storms, which corresponds to stronger geomagnetic disturbance and thus more intense auroral displays.
Statement 5
Can major solar storms (solar flares or coronal mass ejections) directly cause widespread forest fires across large parts of the planet?
Origin: Web / Current Affairs
Fairness: CA heavy
Web-answerable
"In an extreme event in 1859, a large solar eruption triggered a geomagnetic storm that sparked fires in telegraph offices across the United States and triggered aurorae as far south as Central America."
Why this source?
- Documents a historical extreme event (1859) in which a geomagnetic storm 'sparked fires' in telegraph offices — showing solar storms can ignite electrical/industrial fires.
- The passage frames effects as damage to infrastructure (telegraph fires, power-grid destruction) rather than direct ignition of natural landscapes like forests.
"Coronal Mass Ejections (CMEs) can cause Geomagnetic Storms at Earth and induce extra currents in the ground that can degrade power grid operations."
Why this source?
- Explains a mechanism by which CMEs cause geomagnetic storms that 'induce extra currents in the ground that can degrade power grid operations' — a pathway to infrastructure fires or outages.
- Supports the idea that impacts are primarily on technological systems (power grids, satellites, radio), not direct ignition of widespread forests.
"CMEs can cause large geomagnetic storms that affect terrestrial systems such as electric power grids."
Why this source?
- States CMEs 'can cause large geomagnetic storms that affect terrestrial systems such as electric power grids', reinforcing that main impacts are on electrical infrastructure.
- Adds to evidence that solar storms affect man-made systems rather than directly causing large-scale natural fires.
Physical Geography by PMF IAS, Manjunath Thamminidi, PMF IAS (1st ed.) > Chapter 5: Earths Magnetic Field (Geomagnetic Field) > Geomagnetic Storms > p. 68
Strength: 5/5
“• Solar activity drives the space weather (varying conditions in the magnetosphere). If the solar wind is weak, the magnetosphere expands, if it is strong, it compresses the magnetosphere & more of it gets in.• Periods of intense solar activity, called geomagnetic storms, occur when a coronal mass ejection erupts above the Sun & sends a shock wave through the Solar System. It takes just two days for the shock wave to reach the Earth. At the Earth's surface, a magnetic storm is seen as a rapid drop in the Earth's magnetic field strength.• Ring Current: Ring current is the name given to the large electric current that circles the Earth above its equator during magnetic storms.”
Why relevant
Describes coronal mass ejections producing geomagnetic storms at Earth (arriving in ~2 days) and generating large electric currents around the planet.
How to extend
A student could combine this with basic physics to ask whether induced currents or magnetospheric changes can heat or ignite vegetation at the surface.
Physical Geography by PMF IAS, Manjunath Thamminidi, PMF IAS (1st ed.) > Chapter 5: Earths Magnetic Field (Geomagnetic Field) > A Planet's Magnetic Field Protects its Atmosphere > p. 69
Strength: 5/5
“• As the solar wind approaches a planet that has a well-developed magnetic field (such as Earth, Jupiter and Saturn), the particles are deflected by the magnetosphere, which causes the particles to travel around the planet rather than bombarding the atmosphere or surface. Whereas planets with a weak or non-existent magnetosphere are subject to atmospheric stripping by the solar wind.• Venus, the nearest and most similar planet to Earth in the Solar System, has an atmosphere 100 times denser than our own, with little or no geomagnetic field. This is a strange exception.”
Why relevant
States that a planet's magnetosphere deflects solar wind particles, protecting the atmosphere; planets lacking a strong field are more vulnerable to atmospheric effects.
How to extend
One could compare Earth (with a strong magnetosphere) to bodies without one to judge whether solar particle bombardment is sufficient to reach/heat Earth's surface to ignition levels.
Science ,Class VIII . NCERT(Revised ed 2025) > Chapter 13: Our Home: Earth, a Unique Life Sustaining Planet > 13.3.3 Magnetic field of the Earth > p. 217
Strength: 4/5
“Other particles come from the Sun and are called the solar wind. These particles can be harmful as they can damage the atmosphere, reduce the ozone layer, and let in more harmful UV rays, which can affect life on Earth. Thankfully, the Earth's magnetic field acts like a protective shield. It pushes many of these harmful particles away from the Earth, keeping our atmosphere, and hence life on our planet safe. Earth's unique position in the solar system—allows the presence of liquid water—along with its size, atmosphere, and magnetic field, all help make it a planet where life can emerge and thrive.”
Why relevant
Notes solar wind particles can harm the atmosphere and ozone but that Earth's magnetic field acts as a protective shield keeping life safe.
How to extend
A student could use this to assess whether residual solar-particle effects, after magnetospheric shielding, are likely strong enough at ground level to start widespread fires.
Environment and Ecology, Majid Hussain (Access publishing 3rd ed.) > Chapter 12: Major Crops and Cropping Patterns in India > Biotic: Living > p. 122
Strength: 4/5
“Solar energy: Energy derived from the Sun. Solar wind: Clouds of ionised (charged) gases emitted by the Sun and travelling in all directions from the Sun's surface. Efects on Earth include auroras, disturbance of radio signals, and possible infuences on weather. Solifuction: Gentle down-slope movement of a saturated surface material (soil and regolith), in various climatic regimes, where temperatures are above freezing. Solum: A true soil profle in the pedon, ideally, a combination of A and B horizons. Solution: Te dissolved load of a stream. Specifc humidity: Te mass of water vapour (in grams) per unit mass of air (in kilograms) at any specifed temperature.”
Why relevant
Lists known terrestrial effects of solar wind (auroras, radio disturbances, possible influences on weather), implying typical impacts are electromagnetic or atmospheric rather than direct ignition.
How to extend
Compare these common effects with the physical requirements for ignition (temperature, energy delivery) to judge plausibility of direct fire-starting by solar storms.
Physical Geography by PMF IAS, Manjunath Thamminidi, PMF IAS (1st ed.) > Chapter 25: Thunderstorm > Pyrocumulonimbus Clouds And Forest Fires > p. 353
Strength: 3/5
“• The pyrocumulonimbus clouds are essentially thunderstorms (cumulonimbus clouds) that form from the smoke plume of fire as intense heat from the fire causes air to rise rapidly, drawing in the surrounding air. As the cloud climbs and then cools in the low temperatures of the upper atmosphere, the collisions of ice particles in the higher parts of the cloud build up an electrical charge, which can be released as lightning, which could ignite new fires.• The rising air also spurs intense updrafts that suck in so much air that strong winds develop, causing a fire to burn hotter and spread further.• The forest fires in Australia, Western Canada, and California in recent times were accentuated by the formation of pyrocumulonimbus clouds due to severe heat waves.”
Why relevant
Explains pyrocumulonimbus clouds and lightning generated by intense fires, showing a mechanism where fires produce further ignitions via atmospheric processes — i.e., fires can spread by their own induced weather.
How to extend
Use this to distinguish between (a) solar storms directly igniting vegetation and (b) fires spreading through fire-generated weather once started by terrestrial causes.
Statement 6
Can major solar storms (solar flares or coronal mass ejections) disturb satellite orbits by increasing atmospheric drag or causing other orbital perturbations?
Origin: Direct from books
Fairness: Straightforward
Book-answerable
From standard books
Physical Geography by PMF IAS, Manjunath Thamminidi, PMF IAS (1st ed.) > Chapter 5: Earths Magnetic Field (Geomagnetic Field) > Effects of Geomagnetic Storms > p. 68
Presence: 5/5
“• The ionosphere gets heated & distorted, which means that long-range radio communication that is dependent upon sub-ionospheric reflection can be difficult.• Ionospheric expansion can increase satellite drag, and it may become difficult to control their orbits.• Geomagnetic storms disrupt satellite communication systems like GPS.• Astronauts would face high radiation levels.• Electric power grids would see a high increase in voltage that would cause blackouts.”
Why this source?
- Directly states that ionospheric expansion can increase satellite drag.
- Explicitly links geomagnetic/ionospheric disturbance to difficulty in controlling satellite orbits and to disruptions in satellite communications.
Physical Geography by PMF IAS, Manjunath Thamminidi, PMF IAS (1st ed.) > Chapter 20: Earths Atmosphere > Exosphere (700 to 1,000 km) > p. 280
Presence: 4/5
“• The high earth orbit and mid earth orbit satellites are all in the exosphere because the air is so thin that satellites can easily move with little atmospheric drag.”
Why this source?
- Identifies that high- and mid-Earth orbit satellites occupy the exosphere where atmospheric drag is normally minimal.
- Implicates that changes in atmospheric density at those heights (i.e., expansion) would alter the normally low-drag environment and affect orbits.
Physical Geography by PMF IAS, Manjunath Thamminidi, PMF IAS (1st ed.) > Chapter 2: The Solar System > Solar Flares > p. 25
Presence: 3/5
“• Solar are magnetic storms which appear to be very bright spots with a gaseous surface eruption. As solar flares are pushed through the corona, they heat its gas to anywhere from 10 to 20 million °C.”
Why this source?
- Describes solar flares as intense, high-temperature eruptions, providing the energetic source that can heat and perturb the upper atmosphere.
- Supports the mechanism by which solar activity can drive atmospheric heating and expansion that lead to increased drag.
Statement 7
Can major solar storms (solar flares or coronal mass ejections) interrupt shortwave/HF radio communications for aircraft flying over polar regions?
Origin: Direct from books
Fairness: Straightforward
Book-answerable
From standard books
Physical Geography by PMF IAS, Manjunath Thamminidi, PMF IAS (1st ed.) > Chapter 5: Earths Magnetic Field (Geomagnetic Field) > Geomagnetic Storms > p. 68
Presence: 4/5
“• Solar activity drives the space weather (varying conditions in the magnetosphere). If the solar wind is weak, the magnetosphere expands, if it is strong, it compresses the magnetosphere & more of it gets in.• Periods of intense solar activity, called geomagnetic storms, occur when a coronal mass ejection erupts above the Sun & sends a shock wave through the Solar System. It takes just two days for the shock wave to reach the Earth. At the Earth's surface, a magnetic storm is seen as a rapid drop in the Earth's magnetic field strength.• Ring Current: Ring current is the name given to the large electric current that circles the Earth above its equator during magnetic storms.”
Why this source?
- Describes that coronal mass ejections (CMEs) and solar activity drive space weather and produce geomagnetic storms.
- States geomagnetic storms cause rapid changes in Earth's magnetic field and disturb the near‑Earth space environment.
Physical Geography by PMF IAS, Manjunath Thamminidi, PMF IAS (1st ed.) > Chapter 20: Earths Atmosphere > Ionosphere (80 to 400 km) > p. 278
Presence: 5/5
“• Ionosphere is a part of the thermosphere. It extends between 80-400 km. In the ionosphere, Extreme UltraViolet (EUV) and x-ray solar radiation ionize the atoms and molecules thus creating a layer of electrons. The ionosphere is important because it reflects and modifies radio waves used for communication and navigation.• As the radio signal is transmitted, some signals (greater than critical angle or frequency) will escape the earth through the ionosphere (green arrow). The ground wave (purple arrow) is the direct signal or ground wave. This wave weakens quickly due to high energy losses and is what one hears as a fading signal.• The remaining waves (red and blue arrows) are called "skywaves." These waves bounce off the ionosphere and can bounce for many thousands of miles depending upon the atmospheric conditions.”
Why this source?
- Explains the ionosphere is formed by solar EUV/X‑ray radiation producing free electrons.
- Makes clear the ionosphere reflects and modifies radio waves used for communication and navigation (i.e., HF/shortwave skywave propagation).
Certificate Physical and Human Geography , GC Leong (Oxford University press 3rd ed.) > Chapter 2: The Earth's Crust > Great Circle Routes > p. 15
Presence: 3/5
“Firstly, air routes must link numerous cities and thus planes proceed in short 'hops' from place to place; secondly, it may be impossible to fly along great circles for political reasons if some countries forbid the use of their air-space; thirdly, air routes tend to follow the land in case of accident and rarely fly for long distances over the sea. However, where long distances have to be covered over uninhibited regions, great circle routes are the quickest. They are therefore used in crossing polar regions”
Why this source?
- Notes long‑distance air routes commonly use great circle tracks that cross polar regions.
- Establishes that aircraft frequently operate over polar regions where ionospheric conditions are operationally relevant.
Pattern takeaway:
UPSC frequently mixes real scientific phenomena with 'Hollywood Disaster' tropes. If a statement implies a change in the physical state of the solid Earth (Lithosphere) or Ocean (Hydrosphere) directly from a space weather event, be highly skeptical unless it is an asteroid impact.
How you should have studied
- [THE VERDICT]: Conceptual Trap + Applied Science. The trap is the 'Doomsday Fallacy'—assuming a major disaster causes every bad thing imaginable. Source: PMF IAS (Geomagnetism) + General Science logic.
- [THE CONCEPTUAL TRIGGER]: Solar-Terrestrial Interactions. Specifically, the distinction between Solar Flares (Flash/X-rays) and Coronal Mass Ejections (Plasma/Particles) and how they interact with Earth's Magnetosphere.
- [THE HORIZONTAL EXPANSION]: Memorize the NOAA Space Weather Scales: R-Scale (Radio Blackouts - affects HF Comms), S-Scale (Solar Radiation - affects Astronauts/Satellites), G-Scale (Geomagnetic Storms - affects Power Grids/Pipelines). Know that 'G-storms' cause atmospheric expansion (Satellite Drag).
- [THE STRATEGIC METACOGNITION]: Apply the 'Energy Modality Filter'. Solar storms carry electromagnetic and particle energy. Ask: Can charged particles push the ocean floor (Tsunami)? No. Can they thermally ignite wet forests globally? No. Can they induce currents in long wires (Power grids)? Yes.
Concept hooks from this question
👉 Geomagnetic storms and disruption of satellite navigation
💡 The insight
Geomagnetic storms can disrupt satellite communications and GPS by altering the near-Earth electromagnetic environment.
High-yield for questions on space weather impacts, technology vulnerability, and disaster/critical infrastructure management. Connects physical geography (magnetosphere) with applied topics like navigation, communications, and national security; useful for cause–effect and policy-impact questions.
📚 Reading List :
- Physical Geography by PMF IAS, Manjunath Thamminidi, PMF IAS (1st ed.) > Chapter 5: Earths Magnetic Field (Geomagnetic Field) > Effects of Geomagnetic Storms > p. 68
- Environment and Ecology, Majid Hussain (Access publishing 3rd ed.) > Chapter 12: Major Crops and Cropping Patterns in India > Biotic: Living > p. 122
🔗 Anchor: "Can major solar storms (solar flares or coronal mass ejections) disrupt or disab..."
👉 Solar wind as the driver of space weather
💡 The insight
The solar wind is a stream of energetic charged particles that produces geomagnetic storms affecting Earth systems.
Important for understanding mechanisms behind solar-terrestrial interactions, auroras, and technological disruptions. Links to topics on magnetosphere, ionosphere, and their role in communications and satellite operations; enables questions on mitigation and monitoring strategies.
📚 Reading List :
- Physical Geography by PMF IAS, Manjunath Thamminidi, PMF IAS (1st ed.) > Chapter 2: The Solar System > Solar Wind > p. 24
- Physical Geography by PMF IAS, Manjunath Thamminidi, PMF IAS (1st ed.) > Chapter 5: Earths Magnetic Field (Geomagnetic Field) > Bow Shock > p. 66
🔗 Anchor: "Can major solar storms (solar flares or coronal mass ejections) disrupt or disab..."
👉 Ionospheric heating, expansion and satellite drag
💡 The insight
Ionospheric heating and expansion during storms alters radio propagation and increases satellite drag, complicating orbit control and navigation accuracy.
Useful for technical-impact questions on satellites and GPS reliability, and for connecting physical processes to operational challenges in space technology and civil aviation. Supports answers on vulnerability assessment and resilience measures for space-based services.
📚 Reading List :
- Physical Geography by PMF IAS, Manjunath Thamminidi, PMF IAS (1st ed.) > Chapter 5: Earths Magnetic Field (Geomagnetic Field) > Effects of Geomagnetic Storms > p. 68
- Physical Geography by PMF IAS, Manjunath Thamminidi, PMF IAS (1st ed.) > Chapter 2: The Solar System > Solar Wind > p. 24
🔗 Anchor: "Can major solar storms (solar flares or coronal mass ejections) disrupt or disab..."
👉 Primary physical causes of tsunamis
💡 The insight
Tsunamis are generated by large, rapid displacements of water due to earthquakes, volcanic eruptions, landslides and similar major disturbances.
High-yield for questions on coastal hazards and disaster management; links plate tectonics, volcanic activity and slope stability to tsunami risk and mitigation. Enables answers on source mechanisms, risk zones (subduction margins) and historical case studies.
📚 Reading List :
- Physical Geography by PMF IAS, Manjunath Thamminidi, PMF IAS (1st ed.) > Chapter 15: Tsunami > 15. Tsunami > p. 191
- Physical Geography by PMF IAS, Manjunath Thamminidi, PMF IAS (1st ed.) > Chapter 11: Volcanism > 11.10. Destructive Effects of Volcanoes > p. 159
- Geography of India ,Majid Husain, (McGrawHill 9th ed.) > Chapter 17: Contemporary Issues > Causes > p. 15
🔗 Anchor: "Can major solar storms (solar flares or coronal mass ejections) cause tsunamis i..."
👉 Solar activity and geomagnetic storms (CMEs and solar flares)
💡 The insight
Solar flares and coronal mass ejections drive geomagnetic storms by sending shocks and charged particles that affect Earth's magnetosphere.
Important for space weather and its impacts on technology and the magnetosphere; helps distinguish between electromagnetic/ionospheric hazards and oceanic/tectonic hazards, a recurring UPSC theme linking astronomy, environment and infrastructure vulnerability.
📚 Reading List :
- Physical Geography by PMF IAS, Manjunath Thamminidi, PMF IAS (1st ed.) > Chapter 5: Earths Magnetic Field (Geomagnetic Field) > Geomagnetic Storms > p. 68
- Physical Geography by PMF IAS, Manjunath Thamminidi, PMF IAS (1st ed.) > Chapter 2: The Solar System > Solar Flares > p. 25
🔗 Anchor: "Can major solar storms (solar flares or coronal mass ejections) cause tsunamis i..."
👉 Tsunami wave characteristics and propagation
💡 The insight
Tsunamis have very long wavelengths, high energy, and speeds tied to ocean depth, affecting how and where they become destructive.
Useful for answering questions on early warning, coastal vulnerability, and differential impacts in deep vs shallow water; connects physical geography concepts to practical disaster response and planning.
📚 Reading List :
- Environment and Ecology, Majid Hussain (Access publishing 3rd ed.) > Chapter 8: Natural Hazards and Disaster Management > Characteristics of Tsunami Waves > p. 33
- Physical Geography by PMF IAS, Manjunath Thamminidi, PMF IAS (1st ed.) > Chapter 15: Tsunami > 15. Tsunami > p. 190
🔗 Anchor: "Can major solar storms (solar flares or coronal mass ejections) cause tsunamis i..."
👉 Geomagnetic storms and coronal mass ejections (CMEs)
💡 The insight
CMEs drive geomagnetic storms that produce large-scale changes in Earth's magnetic environment and circulating electric currents.
High-yield for UPSC geography and space-weather related disaster management questions: explains the source mechanism of large space-weather events and connects to impacts on technological systems. Mastering this helps answer questions on solar-terrestrial interactions, timelines of CME arrival, and their role in magnetospheric disturbances.
📚 Reading List :
- Physical Geography by PMF IAS, Manjunath Thamminidi, PMF IAS (1st ed.) > Chapter 5: Earths Magnetic Field (Geomagnetic Field) > Geomagnetic Storms > p. 68
- Physical Geography by PMF IAS, Manjunath Thamminidi, PMF IAS (1st ed.) > Chapter 2: The Solar System > Solar Wind > p. 24
🔗 Anchor: "Can major solar storms (solar flares or coronal mass ejections) damage power gri..."
The 'Internet Apocalypse' vulnerability: While fiber optic cables themselves are immune to solar storms (glass doesn't conduct), the copper-based electronic repeaters on long-distance undersea cables are vulnerable to Geomagnetically Induced Currents (GIC), potentially causing global internet isolation.
Use 'Domain Separation' Logic. Solar Storms operate in the Magnetosphere/Ionosphere domain. Tsunamis operate in the Lithosphere/Hydrosphere domain. There is no direct physical mechanism for solar wind to displace ocean water. Eliminate Statement 2 (Tsunamis). This single move eliminates Options A, B, and D, leaving C as the only possible answer.
Mains GS-3 (Disaster Management & Security): Solar storms are a 'Black Swan' threat to Critical Infrastructure. Link this to the vulnerability of 'Cyber-Physical Systems' and the strategic need to harden power grids against EMPs (Electromagnetic Pulses), which mimic the effects of a severe solar storm.