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www.scvemc.org Title : The Lightning Phenomenon Guest Speaker : Marcos Rubinstein (DL) Abstract: Lightning is one of the primary causes of damage and malfunction of telecommunication and power networks and one of the leading causes of


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www.scvemc.org Title : The Lightning Phenomenon Guest Speaker : Marcos Rubinstein (DL)

Abstract: Lightning is one of the primary causes of damage and malfunction of telecommunication and power networks and one of the leading causes of weather-related deaths and injuries. Lightning is composed of numerous physical processes, of which only a few are visible to the naked eye. This lecture presents various aspects of the lightning phenomenon, its main processes and the technologies that have been developed to assess the parameters that are important for engineering and scientific applications. These parameters include the channel-base current and its associated electromagnetic fields. The measurement techniques for these parameters are intrinsically difficult due to the randomness of the phenomenon and to the harsh electromagnetic environment created by the lightning itself. Besides the measurement of the lightning parameters, warning and insurance applications require the real-time detection and location of the lightning strike point. The main classical and emerging lightning detection and location techniques, including those used in currently available commercial lightning location systems will be described in the lecture. The newly proposed Electromagnetic Time Reversal technique, which has the potential to revolutionize lightning location will also be presented.

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The Lightning Phenomenon

Marcos Rubinstein

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Outline

N

What is lightning and the main lightning processes

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How are its parameters measured

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Lightning detection and location

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What is lightning?

Li Lightni ning ng is a a trans ansien ent, hi high-cur curren ent el elect ectric c di dischar charge e who hose e pa path h leng ength h is me measured in kilome meters

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SLIDE 5

Lightning Effects

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About 30%-60% of all power outages annually are lightning-related, on average, with total costs approaching $1 billion dollars. (Source: EPRI)

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Lightning strikes cost nearly $1 billion in insured losses in 2012 (source: Insurance Information Institute)

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SLIDE 6

Kamatzu Airforce Base, Japan

Lightning initiation by an aircraft

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Kamatzu Airforce Base, Japan

Lightning initiation by an aircraft

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SLIDE 8

Cattle Killed by Step or Touch Potential

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A complete lightning is called a “lightning flash”

Major Types of Lightning

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Types of Cloud-to-Ground lightning

Both of these types can transfer either positive or negative charge to the ground.

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Cloud-to-Ground Lightning

Downward negative Upward negative Downward positive Upward positive

Adapted from Berger, 1977

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Downward negative Upward negative Downward positive

Upward positive

About 90% or more of global Cloud-to-ground lightning

Cloud-to-Ground Lightning

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Downward negative Upward negative Downward positive

Upward positive

About 10% or less of global Cloud-to-ground lightning

Cloud-to-Ground Lightning

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Downward negative Upward negative Downward positive Upward positive

Occur only from tall objects (>100 m or so) or from

  • bjects of moderate height

located on mountain tops

Cloud-to-Ground Lightning

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SLIDE 15

Cloud-to-Ground Lightning

Adapted from Berger, 1977

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Separation of charge

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SLIDE 17

Separation of charge

Graupel

+

  • 15o C (~6 km)

_

+

_

Ice crystals

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Cloud-to-Ground Lightning

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Cloud-to-Ground Lightning

Downward negative Upward negative Downward positive Upward positive

Adapted from Berger, 1977

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Downward negative Upward negative Downward positive Upward positive

Cloud-to-Ground Lightning

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Downward Negative Cloud-to-Ground Lightning

Stepped leader

+ +

+ + + + + +

  • - -
  • -
  • +

+ + + + + +

  • - -
  • -
  • +

+ +

  • time

+ +

+ + + + + + + +

  • - -
  • -
  • +

t = 0 Preliminary discharge

+

+ + + + + + +

  • - -
  • -
  • t = 1 ms

+ +

+ + + + + +

  • - -
  • -
  • +

+ +

t = 1.2 ms Upward connecting discharges Attachment process First return stroke

+

  • + +

+

  • -

+

  • -
  • +

++ + + + + + + + + + + +

time

+

  • + +

+

  • -
  • t = 19 ms

+

  • ++

+

  • -
  • +
  • -
  • t = 20 ms

+

  • ++

+

  • -

+

  • +

+ + +

t = 20.1 ms

  • +
+ +
  • +
+ +
  • +
  • +

+ + + +

  • +

+ + +

Dart leader Subsequent return stroke time

+
  • +
+ +
  • t = 60 ms
  • +

+ + +

  • t = 62 ms

Adapted from Uman, 1987

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SLIDE 22

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High speed video (7,200 images per second) of a negative ground flash captured on August 15, 2008 near Rapid City, South Dakota

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SLIDE 23

The three processes we saw in the video

❖ Preliminary breakdown ❖ Stepped Leader ❖ Attachment process ❖ Return stroke ❖ Continuing current ❖ M components ❖ Inter-stroke processes (K and J changes)

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SLIDE 24

There are other processes in downward CG lightning

❖ Preliminary breakdown ❖ Stepped Leader ❖ Attachment process ❖ Return stroke ❖ Continuing current ❖ M components ❖ Inter-stroke processes (K and J changes)

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SLIDE 25

Typical Channel-Base Current Waveform Associated with a Downward Negative Flash

I

First Return Stroke Subsequent Return Stroke Subsequent Return Stroke M Components M Component

CC

t

Tens to hundreds of ms Of the order of a hundred µs Of the order of a hundred µs First RS ~ 30 kA Subsequent RS ~ 12 kA CC ~ tens to hundreds of A M- comp. ~ hundreds of A

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SLIDE 26

Lightning is a Very Long Antenna

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Lightning Return-Stroke Fields: 1-5 km

Typical vertical electric field intensity (left column) and azimuthal magnetic flux density (right column) waveforms for first (solid line) and subsequent (dashed line) return strokes at distances of 1, 2 and 5 km. Adapted from Lin et al. (1979).

Solid Line: First Strokes Dashed Line: Subsequent Strokes

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SLIDE 28

Lightning Return-Stroke Fields: 10-200 km

Typical vertical electric field intensity (left column) and azimuthal magnetic flux density (right column) waveforms for first (solid line) and subsequent (dashed line) return strokes at distances of 10, 15, 50, and 200 km. Adapted from Lin et al. (1979).

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SLIDE 29

Upward Lightning

❖ Only from tall objects or from moderate height objects on mountains ❖ It is becoming more frequent ❖ Above a certain height, tall structures produce their own lightning

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SLIDE 30

Upward Lightning

Upward negative Upward positive

Adapted from Berger, 1977

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High-Speed Video of Upward Lightning

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Upward Negative Lightning

I

Return Stroke Return Stroke ICC pulses M Component

CC

t

CC ICC

Tens to hundreds of ms Of the order of a hundred µs

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SLIDE 33

How are Lightning Measurements Made, Given its Inherent Randomness and Harsh EM environment?

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Direct Channel-Base Measurements

❖ Artificially initiated lightning ❖ Rocket-triggered ❖ Laser triggered? ❖ Instrumented tall grounded objects ❖ Towers, buildings, wind turbines

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Rocket-Triggered Lightning

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Camp Blanding, Florida

Launcher Rockets

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Camp Blnding, Florida

  • F. Rachidi and C.A. Nucci, 2005

36

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SLIDE 37

Tall Grounded Objects

Slide courtesy of Prof. V. Rakov 37

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Instrumented Towers Around the World

Slide courtesy of Prof. V. Rakov 38 2502 m ASL 124 m Morro do Cachimbo 60 m 1430 m ASL Gaisberg 1288 m ASL 100 m Eagle Nest 2537 m ASL 25 m Peissenberg CN Tower Skytree 940 m ASL 76 m ASL 37 m ASL 160 m 553 m 634 m Säntis

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SLIDE 39

39 Säntis mountain: 2502 m; Säntis Tower: 123.5 m

  • Instrumented in May 2010
  • The highest lightning incidence (100+

times a year).

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SLIDE 40

control room

B-dot sensors 82 m 24 m Rogowski coils

Säntis mountain: 2502 m; Säntis Tower: 123.5 m

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SLIDE 41

EMC Box Design

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SLIDE 42

Equipment Installation

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Flat-Plate Sensor for Electric Fields

46 Cut-out disk Metallic box

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Cross-Loop Magnetic Field Sensor

47

NS EW

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SLIDE 45

Electric and Magnetic Fields

Slide courtesy of Prof. V. Rakov 48 Flate-plate antenna (vertical E-field) Two loop antennas (Horizontal H-field)

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SLIDE 46

How is Lightning Located?

49

❖ Well-known (patented) Time-to-Thunder ❖ Direction Finding (DF) ❖ Time of Arrival (TOA) ❖ Interferometry ❖ Peak Amplitude Method ❖ Field Component Methods ❖ Time reversal

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SLIDE 47

Time to Thunder

50

d = Number of seconds × Speed of sound

Light T h u n d e r

The light is 1 million times faster than sound

d = Number of seconds 3 km

𝑒 = 𝑂𝑣𝑛𝑐𝑓𝑠 𝑝𝑔 𝑡𝑓𝑑𝑝𝑜𝑒𝑡 5 𝑁𝑗𝑚𝑓𝑡

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SLIDE 48

Time to Thunder

51

❖ Advantages: ❖ Can be used as single station ❖ It does not require any special equipment ❖ Disadvantages: ❖ Low accuracy ❖ Limited range

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SLIDE 49

Direction Finding

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The radiated magnetic field is perpendicular to the direction of propagation

H E

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SLIDE 50

Direction Finding

53

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Time of Arrival (ToA or DToA)

54

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SLIDE 52

55

Sensor 1

ToA

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Commercial LLS sensor

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GPS Antenne Rahmenspulen

GPS antenna

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European Cooperation for Lightning Detection

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www.euclid.at

  • ca. 164 Sensors (2019)

IMPACT 181T IMPACT ES IMPACT ESP LPATS III LPATS IV LS 7000

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SLIDE 55

Emerging LLS Technology: Time Reversal

58

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Time Reversal Invariance

❖ It is the property of some laws of physics to remain invariant under the T-

Symmetry Transformation

❖ The T-Symmetry Transformation:

59

T :t → −t

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SLIDE 57

Time-reversal Invariance of Maxwell’s Equations

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∇⋅ ε( r )  E( r,t)

( ) = ρ(

r,t) ∇⋅ µ( r )  H( r,t)

( ) = 0

∇ ×  E( r,t) = −µ( r) ∂  H( r,t) ∂t ∇ ×  H( r,t) = ε( r ) ∂  E( r,t) ∂t +  J( r,t)

  • Maxwell’s equations in vacuum are time-reversal invariant
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SLIDE 58

EMTR and Lightning Location

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❖ Record magnetic field at sensors

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  • Time-reverse the measured field
  • Transmit the time-reversed waveforms back into the

medium by simulation

  • Find the point of maximum constructive interference
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SLIDE 59

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Thank you for your Attention!

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