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PLASTIC STEREO SC/B Magnetosheath Observations Lynn M. Kistler Space Science Center UNH

STEREO SC/B Magnetosheath Observations

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STEREO SC/B Magnetosheath Observations. Lynn M. Kistler Space Science Center UNH. S/C B During February, 2007. Z. Y. X. X. Mass - Mass per Charge Matrices All Energies (

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Page 1: STEREO SC/B Magnetosheath Observations

PLASTIC

STEREO SC/B Magnetosheath Observations

Lynn M. KistlerSpace Science Center

UNH

Page 2: STEREO SC/B Magnetosheath Observations

PLASTICS/C B During February, 2007

Y

X

Z

X

Page 3: STEREO SC/B Magnetosheath Observations

PLASTIC

Mass - Mass per Charge MatricesAll Energies (<80 keV)

Feb 10 Feb 11

Feb 12 Feb 13

O+ O+

P0 P1

P2

P3

Page 4: STEREO SC/B Magnetosheath Observations

PLASTIC

Mass - Mass per Charge MatricesFeb 13, 2007

Individual Energies

79 keV/e 59 keV/e

40 keV/e 29 keV/e

P0 P1

P2

P3

Page 5: STEREO SC/B Magnetosheath Observations

PLASTICDensity Calculation

S/CA H+ (SW)

S/C B H+ (Magnetosheath)

S/C A Priority 3 (SW)

S/C B Priority 3 (M-Sheath)

S/CA Priority 3 (1-hr averages)

S/C B Priority 3 (1-hr averages)(this is the O+)

Feb 10 Feb 21

Page 6: STEREO SC/B Magnetosheath Observations

PLASTICDensity Calculation

S/CA H+ (SW)

S/C B H+ (Magnetosheath)

S/C A Priority 3 (SW)

S/C B Priority 3 (M-Sheath)

S/CA Priority 3 (1-hr averages)

S/C B Priority 3 (1-hr averages)

Feb 1 Mar 1

Page 7: STEREO SC/B Magnetosheath Observations

PLASTICSummary

• In the dusk-side magnetosheath, we observe bursts of energetic (30-80 keV) O+

• The O+ correlates with times of high solar wind velocity.

• It is observed as far as 300 Re down the tail.

Page 8: STEREO SC/B Magnetosheath Observations

PLASTICCassini Earth Flyby

-400

-300

-200

-100

0

100

200-500-400-300-200-1000100

Cassini Earth Swingby Trajectory

R*cos(phi) (Re)

August 1999

plotted: 7/13/00

Sun

Earth

230 00:00

12:00

231 00:0012:00

23200:00

12:00 C/A 23003:28 UT

phi = (LT-12)*360/24

End MS232 02:30

Last MP230 10:47 BS

230 01:51

MP

BS

BS and MP fromHowe and Binsack, 1972

From Doug Hamilton

Page 9: STEREO SC/B Magnetosheath Observations

PLASTICCASSINI/CHEMS Magnetosheath Data

1

10

100

230:00:00:00 231:00:00:00 232:00:00:00

Cassini MIMI/CHEMS Earth Flyby

M/Q - Tel 1M/Q - Tel 2M/Q - Tel 3C/A, MP

1999 (UT)

Step 23-29 (73-167 keV/e)Triple coincidence events only

plotted: 12/13/00

X (gse)Y(gse)Z(gse)

31.75.21.2

-70.6-33.0-2.3

-368-167-11.5

-169-79.3-5.4

-268-124-8.4

-468-208-14.6

O+

N+

He+

He ++

H+

Aug. 18 Aug. 19 Aug. 20

O++

C/A MP

Magnetosheath

From Doug Hamilton

Page 10: STEREO SC/B Magnetosheath Observations

PLASTIC

10-2

10-1

100

101

102

103

104

105

106

107

100 101 102

Cassini/MIMI/CHEMS Dawn Tail Sheath

E/Q (keV/e)plotted: 12/13/00

H+

O+

Day 230, 1999 1200-2400

xGSE

= -71 RE to -169 R

E

From Doug Hamilton

Page 11: STEREO SC/B Magnetosheath Observations

PLASTICPossible Sources

• Earth’s Ring Current– Energetic O+ exits the magnetosphere at the dayside

magnetopause, and then gets swept up in the sheath flow

• Upflowing O+ ions from the cusp. – Would they get accelerated enough

• CLUSTER is located at front-side magnetopause/bow-shock - maybe it can see the source - stay tuned ...