Measurement of Atmospheric Electricity During Different Meteorological Conditions
Atmospheric Electricity on Earth and in the Solar System...
Transcript of Atmospheric Electricity on Earth and in the Solar System...
Introduction Thunderstorm Lightning Physics Lightning Observations Lightning Electromagnetic Signatures References
Atmospheric Electricity on Earth and in the Solar SystemEAS 4803/8803: Physics of Planets
Jeremy A. Riousset ([email protected]) Carol S. Paty
School of Earth and Atmopsheric Sciences, Georgia Institute of Technology, Atlanta, GA, USA
October 19, 2011
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Introduction Thunderstorm Lightning Physics Lightning Observations Lightning Electromagnetic Signatures References
Outline
1 Introduction: Global Electrical Circuit
2 The Thunderstorm: Source of the Global Electrical Cir-cuit
3 Lightning Physics
4 Lightning Observations
5 Lightning Electromagnetic Signatures
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Introduction Thunderstorm Lightning Physics Lightning Observations Lightning Electromagnetic Signatures References
Outline
1 Introduction: Global Electrical Circuit
2 The Thunderstorm: Source of the Global Electrical Circuit
3 Lightning Physics
4 Lightning Observations
5 Lightning Electromagnetic Signatures
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Figure: Schematic of various electrical processes in the global electrical circuit [13, p. 6].
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Figure: Role of thunderstorms in the global electrical circuit. Under the thundercloudare precipitation lightning and corona [9, p. 10].
fair weather current ∼1 kA
fair weather conductivity ∼5 × 10−14e
z
8.4 km S/m
fair weather electric field ∼100 V/m
lightning initiation electric field ∼1–2×ez
6 km kV/cm
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Outline
1 Introduction: Global Electrical Circuit
2 The Thunderstorm: Source of the Global Electrical Circuit
3 Lightning Physics
4 Lightning Observations
5 Lightning Electromagnetic Signatures
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Formation and electrification of the cumulonimbus (thundercloud)
∼2000 thunderstorms on Earth at any time [9, p. 10]
≳10% of Earth surface [9, p. 10]
dominant generator in the global circuit [13, p. 6]
Figure: Video courtesy of Dean Gill. Figure: Video courtesy of Daryl Herzmann.
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Thunderstorm cycle
a cumulus stageb mature stagec decaying stage
Figure: Schematic description of a typical cell of an air-mass thunderstorm in threestages of its life cycle. Arrows indicate wind directions. From http://www.noaa.gov/,adapted from [14].
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Thunderstorm electrification
Figure: Schematic of the collisional charging mechanism [9, p. 86].
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Thundercloud electrical structure
Layered structureSize and height vary (e.g., maritime vs continental clouds)Lightning occur every few seconds to every few minutes
Uppernegativecharge
Upperpositivecharge
Mainnegativecharge
Lowerpositivecharge
-25oC-25oC
0oC0oC
Updraft
+ ++ + + ++ + + + +
+ + + + + ++ + + + +
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+ ++ ++ +++ ++ + +++++++ ++ ++ ++ +
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Figure: Schematic of the basic charge structure in the convective region of a thunder-storm [12; 9, p. 83].
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Introduction Thunderstorm Lightning Physics Lightning Observations Lightning Electromagnetic Signatures References
Outline
1 Introduction: Global Electrical Circuit
2 The Thunderstorm: Source of the Global Electrical Circuit
3 Lightning Physics
4 Lightning Observations
5 Lightning Electromagnetic Signatures
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The lightning diversity
Intra-cloud, cloud-to-ground, “cloud-to-ionosphere” (jets), cloud-to-cloud...
Positive or negative
Single or multi-strokes
Stepped or continuous
Figure: (a)–(f) Intracloud, cloud-to-ground, low intracloud, positive blue jet, bolt-from-the-blue, negative gigantic jets. Blue and red contours and numbers indicate negativeand positive charge regions and charge amounts (in C). A partially analogous set ofdischarges occurs or would be predicted to occur in storms having inverted electricalstructures [5].
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Plasma nature of lightning
Bidirectional discharge
Equipotential channel
Overall neutral during propaga-tion
Mostly hot (≳5000 K), highlyconductive
Initiated by high electric field
Reduce charge content in the ap-propriate layers
Leader channel:T>1500 KComplete detachment of negative ionsE~1 kV/cm
Leader corona:Streamer filamentsT~300 KAttached electronsLow conductivityE~5 kV/cm
Transition region:300 K<T<1500 K
Corona front:Active streamer headsHigh space charge fieldAvalanches + photoion-ization
Figure: Sketch of the leader/leader-corona system, withthe main characteristics of the different discharge regions[2].
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Propagation of positive lightning channel [10]
“Natural” lightning = bidirectional system
Positive end simpler than negative end
Positive end usually not visible
Recoil negative event can develop in the positive channel
+U
(a) (b) (c)
(d) (e) (f)
+UE~5 kV/cm
2E~5 kV/cm
E~5 kV/cm
1
3
1 leader tip
2 leader channel
3 streamer zone
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Propagation of negative lightning channel [10]
1 leader tip
2 primary leader channel
3 negative streamers in thestreamer zone
4 space stem or plasma spot
5 negative streamers of thestreamer zone associated withthe negative space leader
6 space leader developing from theplasma spot
7 positive streamers of thestreamer zone associated withthe positive space leader
8 negative end of the space leader
9 positive end of the space leader
10 leader step
11 burst of negative streamers
–U –U
(a) (b) (c)
(d) (e) (f)
(g) (h) (i)
+–
E~ –12.5 kV/cm E~ –12.5 kV/cm
E~ –12.5 kV/cm
E > 5 kV/cm
1
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+–
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+–
+–
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Phenomenology of a –CG [3; 4; 9, p. 110]
1 Intial “stepped” negative leaderdeveloping downward
2 Upward connecting leader
3 Attachment
4 First return stroke
5 “Disconnection” from theground
6 “Dart” continuous leader
7 Second return stroke
8 etc.
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Two –CG captured at 7,207 images per second
Figure: Video courtesy of Tom Warner www.ztresearch.com.
Can you recognize the following features?
Descending stepped leader
Upward connecting leader (why?)
Return stroke
Figure: Video courtesy of Tom Warner www.ztresearch.com.
Can you recognize the following features?
Descending stepped leader
First return stroke
First, second,... dart leaders
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High speed videos of +CG and +GC
A +CG filmed at 7,207 images per second
Figure: Video courtesy of Tom Warner www.ztresearch.com.
Can you recognize the following features?
Descending leaders (weakly luminous)
Bright, short duration recoil leaders onthe weak positive leader channels
Return stroke
A +GC filmed at 7,207 images per second
Figure: Video courtesy of Tom Warner www.ztresearch.com.
Can you recognize the following features?
Ascending leader
Recoil events
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Introduction Thunderstorm Lightning Physics Lightning Observations Lightning Electromagnetic Signatures References
Outline
1 Introduction: Global Electrical Circuit
2 The Thunderstorm: Source of the Global Electrical Circuit
3 Lightning Physics
4 Lightning Observations
5 Lightning Electromagnetic Signatures
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Lightning Mapping Array [11]
Lightning properties:
Wide spectrum
Noisier negative than positive channels
Recoil events in negative channels
Detection method:
Detect 60–66 MHz radiation
Measure TOA at 6 or more stations
Triangulate signal
Products:
3-D time dynamic map of lightning
In and out of the cloud
“Guesstimate” of the polarity of thechannels
-6 -4 -2 0 2 4
-6 -4 -2 0 2 4East-West distance (km)
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19990731
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469 pts
alt-histogram
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Electrical structure of the Cb (part. 2) [8]
Principles:
Channels propagate preferentially in re-gion of higher charge densities
Positive channels propagate in negativeregions
Negative channels propagate in positiveregions
Frequency: several flash/min
Products:
3-D time-integrated electrical structureof the cloud
complements/confirms balloon rocketsoundings
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Balloon and rocket soundings [6; 7]
ρ = ε∆Ez
∆zDo you see any limita-tions?
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Introduction Thunderstorm Lightning Physics Lightning Observations Lightning Electromagnetic Signatures References
Outline
1 Introduction: Global Electrical Circuit
2 The Thunderstorm: Source of the Global Electrical Circuit
3 Lightning Physics
4 Lightning Observations
5 Lightning Electromagnetic Signatures
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Lightning electromagnetic signatures
3 ranges
spherics (or atmospherics): VLF (3–30 kHz)
Schumann resonance: ELF (3 Hz–3 kHz)
whistlers: ELF and VLF (100 Hz –10 kHz)
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Schumann resonance
Resonant spherical cavity [9, p. 452]
TEM wave
λ = R⊕N→ resonance
E = Er(r , ϕ, θ)rB = Bφ(r , ϕ, θ)ϕk = kθ θ
(∇2 + k2)Er = 0
Er,(m,n,l) = (A1jn(kr) +B1nn(kr))´¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¸¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¶spherical Bessel func.
Pmn (cos(θ))´¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¸¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¹¶
assoc. Legendre poly.
(C3 sin(mϕ)+D3cos(mϕ))
[1, p. 557]
fn = c
2πR⊕
√n(n + 1)
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Whistler wave
Figure: Typical path of a ducted whistler within the plasmasphere [9, p. 435].
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Whistler wave
Possible if ω < ωpe = q2nemeε0
, ωce = qB0
me
Ducted by the inner electron belt
High frequencies propagate faster thanlower frequencies → “chirp”
Acoustic frequencies but not in audiblerange
Processed like radio signals from a radiostation
Figure: Courtesy of Donald A. Gurnett, Univ. ofIowa.
http://www-pw.physics.uiowa.edu/plasma-wave/istp/polar/magnetosound.html
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Lightning in the solar system
Schumann resonances [15] and whistlers[9, p. 530] as proxies
Available data for Venus, Jupiter, Sat-urn, Uranus, Neptune [9, p. 530]
Possible electrical discharges on Mars,Titan
What problems do you see?
PlanetType of data Venus Jupiter Saturn Uranus NeptuneOptical ✓ ✓Whistlers ✓ ✓ ✓RF ✓ ✓ ✓ ✓ ✓
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Acknowledgements
Thank You For Your AttentionQuestions?
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References
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[2] D. Comtois, H. Pepin, F. Vidal, F. A. Rizk, C. Y. Chien, T. W. Johnston, J. C. Kieffer, B. La Fontaine, C. Potvin, P. Couture, H. P.Mercure, A. Bondiou-Clergerie, P. Lalande, and I. Gallimberti. Triggering and guiding of an upward positive leader from a ground rodwith an ultrashort laser pulse–II: Modeling. IEEE Trans. Plasma Sci., 31(3):387–395, 2003. doi: 10.1109/TPS.2003.811649.
[3] R. H. Golde. Lightning, volume 1: Physics of Lightning. Academic Press, London, UK; New York, NY, 1977.
[4] R. H. Golde. Lightning, volume 2: Lightning Protection. Academic Press, London, UK; New York, NY, 1977.
[5] P. R. Krehbiel, J. A. Riousset, V. P. Pasko, R. J. Thomas, W. Rison, M. A. Stanley, and H. E. Edens. Upward electrical dischargesfrom thunderstorms. Nature Geoscience, 1(4):233–237, 2008. doi: 10.1038/ngeo162.
[6] T. C. Marshall, W. Rison, W. D. Rust, M. Stolzenburg, J. C. Willett, and W. P. Winn. Rocket and balloon observations of electricfield in two thunderstorms. J. Geophys. Res., 100(D10):20815–20828, 1995. ISSN 0148-0227. doi: 10.1029/95JD01877. URLhttp://dx.doi.org/10.1029/95JD01877.
[7] T. C. Marshall, W. D. Rust, and M. Stolzenburg. Electrical structure and updraft speeds in thunderstorms over the southern greatplains. J. Geophys. Res., 100(D1):1001–1015, 1995. ISSN 0148-0227. URL http://dx.doi.org/10.1029/94JD02607.
[8] T. C. Marshall, M. Stolzenburg, C. R. Maggio, L. M. Coleman, P. R. Krehbiel, T. Hamlin, R. J. Thomas, and W. Rison. Observedelectric fields associated with lightning initiation. Geophys. Res. Lett., 32(3):L03813, 2005. doi: 10.1029/2004GL021802.
[9] V. A. Rakov and M. A. Uman. Lightning: Physics and Effects. Cambridge Univ. Press, Cambridge, U.K.; New York, NY, 2003.
[10] J. A. Riousset. Numerical modeling of lightning, blue jet, and gigantic jets. PhD thesis, The Pennsylvania State University,University Park, PA, August 2010.
[11] W. Rison, R. J. Thomas, P. R. Krehbiel, T. Hamlin, and J. Harlin. A GPS-based three-dimensional lightning mapping system: Initialobservations in central New Mexico. Geophys. Res. Lett., 26(23):3573–3576, 1999. doi: 10.1029/1999GL010856.
[12] M. Stolzenburg, W. D. Rust, and T. C. Marshall. Electrical structure in thunderstorm convective regions–1. Mesoscale convectivesystems. J. Geophys. Res., 103(D12):14059–14078, 1998. doi: 10.1029/97JD03546.
[13] US National Research Council and American Geophysical Union. The Earth’s electrical environment: Based on papers presented atthe American Geophysical Union meetings in June 1983. National Academy Press, Washington, DC, 1986. ISBN 0309036801.Geophysics Study Committee, Geophysics Research Forum, Commission on Physical Sciences, Mathematics, and Resources, NationalResearch Council.
[14] J. M. Wallace and P. V. Hobbs. Atmospheric Science, An Introductory Survey, volume 92 of International Geophysics. AcademicPress, New York, NY, 2nd edition, 1973.
[15] H. Yang, V. P. Pasko, and Y. Yair. Three-dimensional finite-difference time-domain modeling of Schumann resonance parameters onTitan, Venus, and Mars. Radio Sci., 41:RS2S03, 2006. doi: 10.1029/2005RS003431.
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