terrestrial gamma-ray flashes prepared by morris cohen stanford university, stanford, ca ihy...

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Terrestrial gamma-ray flashes Prepared by Morris Cohen Stanford University, Stanford, CA IHY Workshop on Advancing VLF through the Global AWESOME Network

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Page 1: Terrestrial gamma-ray flashes Prepared by Morris Cohen Stanford University, Stanford, CA IHY Workshop on Advancing VLF through the Global AWESOME Network

Terrestrial gamma-ray flashes

Prepared by Morris CohenStanford University, Stanford, CA

IHY Workshop on Advancing VLF through the Global AWESOME

Network

Page 2: Terrestrial gamma-ray flashes Prepared by Morris Cohen Stanford University, Stanford, CA IHY Workshop on Advancing VLF through the Global AWESOME Network

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CGRO designed to study cosmic gamma-raysA number of “surprise” events coming from EarthCGRO locations usually over thunderstormsOnly 75 events observed over 9 years

Short ~1 ms spike in gamma-rays!

Compton Gamma-ray Observatory

Discovery of TGFs by CGRO

Page 3: Terrestrial gamma-ray flashes Prepared by Morris Cohen Stanford University, Stanford, CA IHY Workshop on Advancing VLF through the Global AWESOME Network

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Mesospheric Phenomena

TGFs associated with lightning Observed by gamma-ray detector on spacecraft

Page 4: Terrestrial gamma-ray flashes Prepared by Morris Cohen Stanford University, Stanford, CA IHY Workshop on Advancing VLF through the Global AWESOME Network

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TGF Physical Origins

For energetic electrons, frictional losses in air is a function of energy

Frictional losses reach local minimum near 1 MeV

What if an electric field exists that is larger than this frictional force??

Page 5: Terrestrial gamma-ray flashes Prepared by Morris Cohen Stanford University, Stanford, CA IHY Workshop on Advancing VLF through the Global AWESOME Network

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Step 1: Avalanche Runaway

TGFs formed via four step process Acceleration of electrons due to high

electric fields from lightning More electrons freed due to collisions with

air molecules Relativistic electrons collide with

molecules, release gamma radiation Gamma-rays escape atmosphere

Page 6: Terrestrial gamma-ray flashes Prepared by Morris Cohen Stanford University, Stanford, CA IHY Workshop on Advancing VLF through the Global AWESOME Network

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Avalanche runaway

e-

Electric field

greater than

threshold Air molecule

Air molecule Air

molecule

“seed” electron

Page 7: Terrestrial gamma-ray flashes Prepared by Morris Cohen Stanford University, Stanford, CA IHY Workshop on Advancing VLF through the Global AWESOME Network

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Avalanche runaway

e-

Electric field

greater than

threshold Air molecule

Air molecule Air

molecule

“seed” electron

Acceleration and collision

Page 8: Terrestrial gamma-ray flashes Prepared by Morris Cohen Stanford University, Stanford, CA IHY Workshop on Advancing VLF through the Global AWESOME Network

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Avalanche runaway

Electric field

greater than

threshold Air molecule

Air molecule Air

molecule

e-e-

More electrons freed

Page 9: Terrestrial gamma-ray flashes Prepared by Morris Cohen Stanford University, Stanford, CA IHY Workshop on Advancing VLF through the Global AWESOME Network

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Avalanche runaway

Electric field

greater than

threshold Air molecule

Air molecule Air

molecule

e-e-

More electrons freed

Acceleration and collision again

Page 10: Terrestrial gamma-ray flashes Prepared by Morris Cohen Stanford University, Stanford, CA IHY Workshop on Advancing VLF through the Global AWESOME Network

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Avalanche runaway

Electric field

greater than

threshold Air molecule

Air molecule Air

molecule

e- e-

e- e-

Avalanche continues

Page 11: Terrestrial gamma-ray flashes Prepared by Morris Cohen Stanford University, Stanford, CA IHY Workshop on Advancing VLF through the Global AWESOME Network

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Bremsstrahlung

Air molecule

e-

Relativistic (i.e. close to speed of light) electron collides with air molecule

Electron may lose energy, gamma-ray is emitted

e-

Emitted gamma-ray

Page 12: Terrestrial gamma-ray flashes Prepared by Morris Cohen Stanford University, Stanford, CA IHY Workshop on Advancing VLF through the Global AWESOME Network

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Escaping the atmosphere: Gamma-rays

Gamma-rays may be emitted in many directions Gamma-rays continue straight but may also be

absorbed by molecules Gamma-rays generated high enough (where air

is thin) escape atmosphere more easily

Emitted gamma-rays

Air molecule

Page 13: Terrestrial gamma-ray flashes Prepared by Morris Cohen Stanford University, Stanford, CA IHY Workshop on Advancing VLF through the Global AWESOME Network

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Escaping the atmosphere: Electrons

Do sufficient number of electrons escape? Lower in atmosphere: Collisions too frequent,

electrons cannot escape Higher at atmosphere: Electrons confined to

motion around magnetic field

Air molecule

e- e-

Earth’s magnetic field

Page 14: Terrestrial gamma-ray flashes Prepared by Morris Cohen Stanford University, Stanford, CA IHY Workshop on Advancing VLF through the Global AWESOME Network

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Mechanisms

Figure courtesy Brant Carlson

Lightning generates high electric fields in several different ways

Which process is responsible for accelerating electrons to 0.999c?

Page 15: Terrestrial gamma-ray flashes Prepared by Morris Cohen Stanford University, Stanford, CA IHY Workshop on Advancing VLF through the Global AWESOME Network

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Studying TGFs with ELF/VLF

Peak-VLF ELF tail

Lightning also generates sferic, detectable at long distances

Sferic is also “fingerprint” of lightning Properties of received sferic may help learn

about mechanism of generating TGFs

Page 16: Terrestrial gamma-ray flashes Prepared by Morris Cohen Stanford University, Stanford, CA IHY Workshop on Advancing VLF through the Global AWESOME Network

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TGF from BATSE and VLF

Page 17: Terrestrial gamma-ray flashes Prepared by Morris Cohen Stanford University, Stanford, CA IHY Workshop on Advancing VLF through the Global AWESOME Network

TGF from RHESSI and VLF

Page 18: Terrestrial gamma-ray flashes Prepared by Morris Cohen Stanford University, Stanford, CA IHY Workshop on Advancing VLF through the Global AWESOME Network

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TGF-Lightning Timing

Page 19: Terrestrial gamma-ray flashes Prepared by Morris Cohen Stanford University, Stanford, CA IHY Workshop on Advancing VLF through the Global AWESOME Network

Many types of sferic waveform

Streak of smaller, shorter sferics

Single strong, longer sferic

Page 20: Terrestrial gamma-ray flashes Prepared by Morris Cohen Stanford University, Stanford, CA IHY Workshop on Advancing VLF through the Global AWESOME Network

Multi-burst TGFs

CGRO/BATSERHESSI

Page 21: Terrestrial gamma-ray flashes Prepared by Morris Cohen Stanford University, Stanford, CA IHY Workshop on Advancing VLF through the Global AWESOME Network

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Lightning characteristics

+ + ++ +

++ ++

++ ++ + +

+++

- -- - -- -- ----

-

+ +++++ +

+

Return stroke peak current (i.e., kA)

+ + ++ +

+ ++

++ ++ + +

++

----

-

+ +

Total charge moment (I.e., C•km)

Page 22: Terrestrial gamma-ray flashes Prepared by Morris Cohen Stanford University, Stanford, CA IHY Workshop on Advancing VLF through the Global AWESOME Network

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Peak Current

+ + ++ +

++ ++

++ +

+ + ++++

- -- - -

- -- -

----

+ ++

++

+ +

+

Return stroke peak current (i.e., kA)

Peak current is proportional to VLF peak for a given propagation path

VLF Peak

Page 23: Terrestrial gamma-ray flashes Prepared by Morris Cohen Stanford University, Stanford, CA IHY Workshop on Advancing VLF through the Global AWESOME Network

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Total Charge Moment

Total ELF energy is proportional to total charge transfer

ELF energy attenuates more in Earth-ionosphere waveguide

ELF Energy

+ + ++ +

+ ++

++ ++ + +

++

----

-

+ +

Total charge moment (I.e., C•km)

Reising [1998]

Page 24: Terrestrial gamma-ray flashes Prepared by Morris Cohen Stanford University, Stanford, CA IHY Workshop on Advancing VLF through the Global AWESOME Network

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Regional division

Most TGFs (94%) of TGFs have associated sferics detectable at Palmer Station, Antarctica

Page 25: Terrestrial gamma-ray flashes Prepared by Morris Cohen Stanford University, Stanford, CA IHY Workshop on Advancing VLF through the Global AWESOME Network

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TGF-associated sferics

TGF-associated sferics have high VLF energy High peak current lightning

No high ELF energy Low peak current, unlike

sferics that generate sprites

Page 26: Terrestrial gamma-ray flashes Prepared by Morris Cohen Stanford University, Stanford, CA IHY Workshop on Advancing VLF through the Global AWESOME Network

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TGFs – Research done to date

TGFs occur within a few ms of lightning Tend to be higher peak current Characteristics of lightning do not

resemble those of sprites TGFs likely sourced 15-20 km altitude

(above thunderclouds)

Page 27: Terrestrial gamma-ray flashes Prepared by Morris Cohen Stanford University, Stanford, CA IHY Workshop on Advancing VLF through the Global AWESOME Network

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TGFs – Open questions

Do electrons escape atmosphere along field lines, precipitate at conjugate region?

What lightning processes are chiefly responsible for TGFs?

How often do TGFs occur? Do cosmic ray fluxes affect TGFs?