Notetaker: Space Environment Flashcards

Demarcation, the Sun, Magnetosphere, and Ionosphere (46 cards)

1
Q

Karman Line

A

International Standard
100km (62 miles) above Earth’s surface

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2
Q

USSPACECOM domain

A

U.S. Government Standard
100km (62 miles) above mean sea lvel

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3
Q

Exobase

A

Scientific Community Standard
500 to 1,000 km (310-620 miles) above Earth’s surface

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4
Q

The sun is composed of what?

A
  1. Hydrogen
  2. Helium
  3. Misc Gases
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5
Q

The sun is made of 74.9% of what?

A

Hydrogen

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6
Q

The sun is made of 23.8% of what?

A

Helium

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7
Q

The sun is made of 1.3% of what?

A

Misc gases

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8
Q

The sun creates energy through what?

A

Nuclear Fusion

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9
Q

Core

A

Rotates like a solid and is where fusion occurs

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10
Q

Radiative Zone

A

Rotates like a fluid and radiates energy

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11
Q

Tachocline

A

Generates magnetic field lines and stores magnetic flux

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12
Q

Convective Zone

A

Rotates like a fluid and transfers heat through convection

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13
Q

Photosphere

A

Known as the “surface” and is responsible for 99% of solar radiation

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14
Q

Atmosphere

A

Has 4 sublayers all of which are only visible during an eclipse

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15
Q

What is referred to as “Quiet Sun?”

A

Solar Minimum

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16
Q

Solar Minimum

A
  • Few to zero sunspots
  • Dimmer EUV & x-rays
  • Minimum flaring/CME
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17
Q

What is referred to as “Active Sun?”

A

Solar Maximum

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18
Q

Solar Maximum

A
  • Many sunspots
  • Brighter EUV & x-rays
  • Frequent flaring/CME
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19
Q

Solar Wind

A

A stream of charged particles released from the Corona

20
Q

What solar hazard takes ~3 days to arrive?

21
Q

What causes auroras and the plasma trails on comets?

22
Q

Solar Flare

A

A sudden burst of high energy particles and radiation

23
Q

What solar hazard travels at the speed of light and arrives in ~8 minutes?

24
Q

What is responsible for increased atmospheric drag on LEO, the ionosphere becoming more charged, increased GPS errors, and a source of Radio Blackout Storms?

25
Solar Energetic Particles
High energy particles emanating from the Sun outside the standard solar wind
26
What solar hazard arrival varies from 15 minutes to 24 hours?
Solar Energetic Particles
27
What is responsible for degrading spacecraft components and a source of Radiation Storms?
Solar Energetic Particles
28
Coronal Mass Ejection
A **massive cloud** of energetic, magnetized solar plasma launched into space
29
What solar hazard typically arrives in 3 to 4 days?
Coronal Mass Ejection
30
What can severely disrupt anything that uses electricity (e.g. power grids, satellites, communication networks) and is a main source of Geomagnetic Storms?
Coronal Mass Ejection
31
Earth's Magnetic Field is also known as what?
Geomagnetic Field / Magnetosphere
32
Where the earth interacts with the solar wind and other solar hazards
Magnetosphere
33
What is created by the earth's liquid metal outer core constantly moving?
Magnetosphere
34
What deflects most solar wind?
Magnetosphere
35
# Define: Van Allen Belts
**Trapped charged particles** from the sun
36
What is populated by trapped solar wind electrons?
The Outer Belt
37
What is populated by protons from geomagnetic storms on the earth's night-side?
The Inner Belt
38
What belt is not very stable due to the unpredictability of solar cycle and solar winds?
The Outer Belt
39
What belt is more stable and 10 times more energetic?
The Inner Belt
40
The Ionosphere consists of what?
Plasma (positive ions & free electrons)
41
The Ionosphere is responsible for what?
Scintillation
42
Variations in amplitude, phase, and polarization of signals transmitted through a medium
Scintillation
43
How often does scintillation happen?
Daily ## Footnote Also is very localized
44
Scintillation causes what on satellite communications and GPS positioning?
* Signal fading * Data dropouts
45
The strength of a storm determine what two characteristics of an aurora?
* Intensity * Location
45
The Ionosphere is responsible for northern lights and southern lights, known as what?
* Aurora Borealis (northern) * Aurora Australis (southern) ## Footnote Think of Australia in the south.