l. svalgaard - leif we determine solar wind parameters for... · l. svalgaard easy toolkit, inc....

17
1 How we determine solar wind parameters for the past 150 years. L. Svalgaard Easy Toolkit, Inc. 6927 Lawler Ridge, Houston, TX 77055, USA. ([email protected]) Abstract The solar wind and its embedded interplanetary magnetic field (IMF) buffet the Earth’s magnetosphere resulting in continuous geomagnetic activity, waxing and waning with the changing wind. The very complex phenomenon of geomagnetic activity is described by "geomagnetic indices". Different indices respond with different sensitivities to different parameters of the solar wind; some are most sensitive to changes in the magnetic field, B; some are more sensitive to the solar wind speed, V. By exploiting these different dependencies we can determine both B and V and their possible long-term trends. In particular we find that at at each solar minimum B returns to an almost constant "floor" value of ~4.5 nT, implying that there is no secular trend in the strength of the IMF.

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1

How

we

dete

rmin

e so

lar

win

d pa

ram

eter

s fo

r th

e pa

st 1

50 y

ears

.

L. S

valg

aard

Ea

sy T

oolk

it, In

c.

6927

Law

ler R

idge

, Hou

ston

, TX

770

55, U

SA.

(leif@

leif.

org)

A

bstr

act

The

sola

r w

ind

and

its e

mbe

dded

inte

rpla

neta

ry m

agne

tic f

ield

(IM

F) b

uffe

t the

Ear

th's

mag

neto

sphe

re r

esul

ting

in

cont

inuo

us g

eom

agne

tic a

ctiv

ity, w

axin

g an

d w

anin

g w

ith t

he c

hang

ing

win

d. T

he v

ery

com

plex

phe

nom

enon

of

geom

agne

tic a

ctiv

ity is

des

crib

ed b

y "g

eom

agne

tic in

dice

s". D

iffer

ent i

ndic

es re

spon

d w

ith d

iffer

ent s

ensi

tiviti

es to

di

ffere

nt p

aram

eter

s of

the

sola

r w

ind;

som

e ar

e m

ost s

ensi

tive

to c

hang

es in

the

mag

netic

fie

ld, B

; som

e ar

e m

ore

sens

itive

to th

e so

lar w

ind

spee

d, V

. By

expl

oitin

g th

ese

diffe

rent

dep

ende

ncie

s w

e ca

n de

term

ine

both

B a

nd V

and

th

eir

poss

ible

long

-term

tren

ds. I

n pa

rticu

lar

we

find

that

at a

t eac

h so

lar

min

imum

B r

etur

ns to

an

alm

ost c

onst

ant

"flo

or"

valu

e of

~4.

5 nT

, im

plyi

ng th

at th

ere

is no

secu

lar t

rend

in th

e st

reng

th o

f the

IMF.

2

A

= k

q(a,

f) (B

V) (

n V

2 )1/3 ~

B V

2

3

4

IH

V =

sum

of u

nsig

ned

diffe

renc

es b

etw

een

7 ho

urly

mea

ns c

ente

red

at m

idni

ght

5

10100

1000

-90

-75

-60

-45

-30

-15

015

3045

6075

90

Co

rre

cte

d G

eo

ma

gn

eti

c L

ati

tud

e

IHV (log-scale)

NS

<IH

V>

199

6-20

03

020406080

1960

1961

1962

1963

1964

1965

1966

1967

1968

1969

1970

1971

1972

IHV

IHV

15N

NG

K-F

UR

-WN

G-W

IT-R

SV

-CLF

-HA

D

6

BV

o2 =

4.3

4 (

IHV

- 6

.5)

R2 =

0.7

6

0

10

0

20

0

30

0

40

0

02

04

06

08

01

00

IHV

BV

o2

Ro

tati

on

Me

an

s

050100

150

200

250 19

6519

7019

7519

8019

8519

9019

9520

0020

0

BVo2 (I

HV)

BVo2 (O

bs)

R-C

Effe

ct

7

NH P

ower

(GW

) = 0

.680

7 IH

VR2 =

0.8

582

010203040506070

020

4060

8010

0

1978

-200

6

0102030405060

1978

1980

1982

1984

1986

1988

1990

1992

1994

1996

1998

2000

2002

2004

2006

PO

ES (G

W) N

our

cal

ibra

tion

0.68

* IH

V N

Hem

isph

eric

Pow

er In

put (

PO

ES) a

nd IH

V G

eom

agne

tic A

ctiv

ity

8

ID

V =

Ave

rage

uns

igne

d di

ffere

nce

betw

een

the

mid

nigh

t hou

rly m

eans

from

one

day

to th

e ne

xt.

024681012141618

1870

1880

1890

1900

1910

1920

1930

1940

1950

1960

1970

1980

1990

2000

10u

IDV

(H)

Yea

rly a

vera

ges

B =

0.46

IDV

+ 2.

09R2 =

0.8

7

V/10

0 =

0.03

IDV

+ 4.

14R2 =

0.0

4

B =

0.38

IDV

+ 2.

78R2 =

0.7

9

R2 = 0

.87

024681012

05

1015

20

1965

-200

6

IDV

012345678910

1960

1965

1970

1975

1980

1985

1990

1995

2000

2005

2010

012345678910

B st

d.de

v

Cove

rage

100%

=>

B ob

sB

calc

from

IDV

B ob

s m

edia

n

9

ID

V is

clo

sely

rela

ted

to n

egat

ive

valu

es o

f Dst

: J.

Love

has

cal

cula

ted

Dst

bac

k to

190

5.

IDV

= -0

.40

Dst

(<0)

+ 2

.85

R2 = 0

.89

024681012141618

-40

-30

-20

-10

0

1905

-200

4

IDV

Dst

(<0)

Year

ly a

vera

ges

024681012141618

1870

1880

1890

1900

1910

1920

1930

1940

1950

1960

1970

1980

1990

2000

1909

IDV

IDV

cal

c. fr

om D

st(<

0)

10

024681012

1870

1890

1910

1930

1950

1970

1990

2010

B n

T

Yea

r

IMF

B in

ferre

d fro

m ID

V

B =

0.4

45 ID

V +

2.21

R2 =

0.8

9

012345678910

1870

1880

1890

1900

1910

1920

1930

1940

1950

1960

1970

1980

1990

2000

B n

T

B =

2.78

+ 0

.38

IDV

B =

3.93

- 0.

1546

(Dst

<0)

B IM

F ob

s

IMF

B in

ferr

ed fr

om ID

V an

d Ds

t

11

B =

0.28

82 s

qrt(R

z) +

4.4

856

R2 = 0

.713

9

012345678910

05

1015

B nT

sqrt(

Rz)

1872

-200

6

012345678910

1830

1840

1850

1860

1870

1880

1890

1900

1910

1920

1930

1940

1950

1960

1970

1980

1990

2000

Infe

rred

IMF

B s

ince

183

6B

nT

Year

From

Bar

tels

u-m

easu

reIM

F B

obs

S/C

From

IDV

From

sqr

t(Rz)

12

Po

lar C

ap C

urre

nt S

heet

13

Kin

gua

Fjor

d 18

82-1

883

14

-80

-60

-40

-20020406080100

-100

-80

-60

-40

-20

020

4060

80

BLC

CB

B

ALE

RES

THL

Vect

or V

aria

tion

of H

oriz

onta

l Com

pone

nts

1980

-200

4

15

VB

= 5

0.14

6 R

ES

R2 =

0.8

594

VB

= 5

0.59

7 TH

LR

2 = 0

.885

6

0

1000

2000

3000

4000

5000

020

4060

8010

0

Ampl

itude

(nT)

VB (k

m/s

* nT

)

1965

-200

4

0

1000

2000

3000

4000

5000

1965

1970

1975

1980

1985

1990

1995

2000

2005

VB

(km

/s *

nT

)

Ob

serv

ed

S/C

RE

S (

Re

solu

te B

ay)

TH

L (

Th

ule

)

16

012345678910

1890

1900

1910

1920

1930

1940

1950

1960

1970

1980

1990

2000

B fr

om ID

V

V o fr

om IH

VO

bser

ved

in s

itu

01020304050

1890

1900

1910

1920

1930

1940

1950

1960

1970

1980

1990

2000

BV o

cal

c. fr

om ID

V an

d IH

V

BV o

cal

c. fr

om P

olar

Cap

B

V o o

bser

ved

17

Th

e Fl

oor i

n IM

F B

02468101214

1880

1890

1900

1910

1920

1930

1940

1950

1960

1970

1980

1990

2000

IMF

B In

ferr

ed fr

om ID

V-In

dex

(Rot

atio

n Av

g.)

B o

bsB

= 1

.67

IDV

0.6

nT

Floo

r

01234567 1880

1890

1900

1910

1920

1930

1940

1950

1960

1970

1980

1990

2000

Sola

r Win

d Sp

eed

Infe

rred

from

IHV

and

IDV

V o 1

00 k

m/s

V o o

bsV o

= 1

.6 [(

IHV

- 5) /

IDV

0.6] 1

/2