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Space Weather: The Sun, Magnetosphe re, Ionosphere

Space Weather: The Sun, Magnetosphere, Ionosphere

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Page 1: Space Weather: The Sun, Magnetosphere, Ionosphere

Space Weather:

The Sun, Magnetosphere, Ionosphere

Page 2: Space Weather: The Sun, Magnetosphere, Ionosphere

Source of Space Weather / Ionospheric Disturbances: The Sun

Page 3: Space Weather: The Sun, Magnetosphere, Ionosphere

The Sun:

The Sun for a a couple months in 2001

Facts (approximate values):• 149 million kilometers

away• Diameter: 1.4 million km• Mass: 2.0x1030 kg• 4.5 billion years old• 11 Year sunspot cycle• Surface temp. 5,900 K.• Rotation Period: 27 days

at equator

Page 4: Space Weather: The Sun, Magnetosphere, Ionosphere

Close-up of a Sun Spot

Page 5: Space Weather: The Sun, Magnetosphere, Ionosphere

Local Internal Dynamics

Animation showing our present understanding

Coronal “loops” on the Sun

Page 6: Space Weather: The Sun, Magnetosphere, Ionosphere

Coronal Mass Ejections

Super prominence

EUV images of Sun with corona as observed from SOHO

Page 7: Space Weather: The Sun, Magnetosphere, Ionosphere

Coronal Mass Ejection Causing the Aurora

Page 8: Space Weather: The Sun, Magnetosphere, Ionosphere

Magnetosphere

Other effects include satellite damage, power outages, GPS errors,radio interruptions, etc.

Page 9: Space Weather: The Sun, Magnetosphere, Ionosphere

The Magnetosphere

Page 10: Space Weather: The Sun, Magnetosphere, Ionosphere

The Aurora

As seen from space

As seen in Alaska

Page 11: Space Weather: The Sun, Magnetosphere, Ionosphere

Solar Flares• EUV• X-RAY• “White Light”

Extreme Ultraviolet (EUV)X-ray

Flare

Page 12: Space Weather: The Sun, Magnetosphere, Ionosphere

Troposphere

Stratosphere

Mesosphere

Thermosphere

D-Region

E-Region

F1-Region

F2-Region F2-Region

Neutral Atmosphere Daytime Nighttime

Heig

ht

1

00

km

2

00

km

300

km

Mt. Everest

Page 13: Space Weather: The Sun, Magnetosphere, Ionosphere

Formation of the Ionosphere

EUV Light

Neutral Atoms

PositivelyCharged Ion

Free Electrons, these reflect radio waves

Photo-ionization

SUN

A (Atom) A+ (Ion) + e- (electron)

Photo-ionization occurs when Extreme Ultraviolet (EUV) from the Sun strikes neutral atoms to produce positively charged Ions

Types of Atoms: primarily Oxygen & NitrogenTypes of Molecules: O2, N2, NO

Page 14: Space Weather: The Sun, Magnetosphere, Ionosphere

Two Types of Recombination:

Molecule A2

Ion X+

Charge ExchangeX+ + A2 AX+ + A

AX+ A

Dissociation RecombinationAX+ + e- A + X

oSingleAtom A

Neutral Atom X

Radiative RecombinationX+ + e- A + Radiated Energy

A

Ion X+

e-

Dissociation recombination, 2 steps:

Radiative recombination, 1 step:

Electron splits AX+

apart

Page 15: Space Weather: The Sun, Magnetosphere, Ionosphere

When ions are “let go” they oscillate in simple harmonic motion at an Angular Frequency 2 = N e2 / 0 m

N = Electron Densitye = Charge on electronm = Mass of an electron0 = Permittivity of free space

Angular Plasma Frequency (maximum usable frequency):fN = 2 / fN = Plasma frequency in HertzfN

2 = 80.5 N Substituting Atomic Constants

fc 9 x 10-6 √Nm fc = Critical Frequency,Nm = Electron density

Reflectivity of the Ionosphere

Page 16: Space Weather: The Sun, Magnetosphere, Ionosphere

Electron Density vs. Height

D - Region• 90 Km, Lower following solar

flare• 1.5x104 Ne/cm3 (noon)• Absent at Night

E - Region• 110 Km• 1.5x105 Ne/cm3 (noon)• 1.0x104 Ne/cm3 (Night)

F1 - Region• 200 Km• 2.5x105 Ne/cm3 (noon)• Absent at night

F2 - Region• 300 Km• 106 Ne/cm3 (noon)• 105 Ne/cm3 (Midnight)

Source:“The Ionosphere: Communications, Surveillance, and Direction Finding”

Leo F. McNamara1991ISBN: 0-89464-040-2

Page 17: Space Weather: The Sun, Magnetosphere, Ionosphere

Maximum UseableFrequencyThe Maximum Useable Frequency (MUF) is the largest frequency that can be reflected by the ionosphere at vertical incidence

Source:“The Ionosphere: Communications, Surveillance, and Direction Finding”

Leo F. McNamara1991ISBN: 0-89464-040-2

Page 18: Space Weather: The Sun, Magnetosphere, Ionosphere

Variability of the Ionosphere

• Diurnal (Thru the day)• Seasonal (Thru the year)• Location (Geographic & Geomagnetic)• Solar Activity (Solar Cycles & Disturbances)• Height (at different layers)

Source:“The Ionosphere: Communications, Surveillance, and Direction Finding”

Leo F. McNamara1991ISBN: 0-89464-040-2