[PDF] Top 20 Double Star TC-1 observations of component reconnection at the
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Double Star TC-1 observations of component reconnection at the
... the TC-1 list. These observations provide significant new evidence that reconnec- tion may also take place at the low-latitude dayside magne- topause MP for northward ... See full document
7
Coordinated Cluster/Double Star observations of dayside reconnection signatures
... and TC-1 crosses the magnetopause at high southerly latitudes, further dawnward at ∼08:00 ...and TC-1, ...on TC-1, with the lagged, IMF clock angle at the ...for ... See full document
9
Observations of lion roars in the magnetosheath by the STAFF/DWP experiment on the Double Star TC-1 spacecraft
... “Double Star – First Results” ...the Double Star TC- 1 spacecraft (570 km by 78 970 km, inclination at ...for observations of lion roars as the spacecraft is in the ... See full document
6
Space and ground based investigations of dayside reconnection: Cluster, double star and SuperDARN observations
... Magnetic reconnection was occurring in the vicinity of the sub-solar point during an inter- val of duskward oriented ...the reconnection site and passed over the Double Star and Cluster ... See full document
10
Observation of reconnection pulses by Cluster and Double Star
... As remote sensing of the edge of the plasma sheet boundary occurs, the increases and decreases of the flux intensity of electrons and ions indicate that the satellites are approaching or moving away from the plasma sheet ... See full document
7
Coordinated Cluster/Double Star and ground-based observations of dayside reconnection signatures on 11 February 2004
... in the middle of the figure, where its length has been limited to an arbitrary maximum of 10 R E and the model allows the position relative to the subsolar point to be chosen. Pairs of open reconnected flux tubes are ... See full document
21
Double Star, Cluster, and ground-based observations of magnetic reconnection during an interval of duskward oriented IMF:
... 1 Dept. of Physics & Astronomy, University of Leicester, Leicester LE1 7RH, UK 2 Rutherford Appleton Laboratory, Didcot, Oxfordshire, OX11 0QX, UK 3 Blackett Laboratory, Imperial College, London SW7 2BZ, UK ... See full document
5
Quasi-continuous reconnection accompanied by FTEs during IMF B z 0 nt observed by Double Star TC-1 at the dawnside magnetopause
... In order to verify the occurrence of reconnection, the Walén tests have been carried out at the crossings of the magnetopause current sheet. As illustrated in figure 3 (a~e, with the time intervals, correlations ... See full document
15
Mirror waves and mode transition observed in the magnetosheath by Double Star TC-1
... As MM structures are characterized by compressional power with the fluctuations only in magnetic field magni- tude and not in direction, it is preferable to present the mag- netic field vector in polar coordinates. The ... See full document
5
The large-scale magnetospheric electric field observed by Double Star TC-1
... by Double Star TC-1 data for radial distances ρ between ...sunward component of the electric field decreases monotonically as ρ increases and approaches zero as the distance off the ... See full document
7
Cluster and Double Star observations of dipolarization
... and Double Star (TC- 1) were located in the same local time sector: 7 August 2004, 18:00–24:00 UT, during a disturbed southward/northward IMF interval, and 14 August 2004, 21:00–24:00 UT, when ... See full document
6
Bandwidths and amplitudes of chorus-like banded emissions measured by the TC-1 Double Star spacecraft
... The frequency separation between these two boundaries (full width at half maximum) represents two half widths of each channel. The half widths vary between 10 Hz and 320 Hz. Unfortunately, the solid boom carrying the ... See full document
16
Cluster and Double Star multipoint observations of a plasma bubble
... report observations of one such plasma bubble, made by the four Cluster spacecraft and Double Star TC-2 around 14:00 UT on 21 September 2005, during a period of southward, but B Y -dominated ... See full document
19
Cluster multispacecraft observations at the high-latitude duskside magnetopause: implications for continuous and component magnetic reconnection
... magnetic reconnection During about four hours the Cluster spacecraft, separated by a distance of a few thousands kilometers, observe anoma- lous flows, ...magnetic reconnection, as shown by the satisfactory ... See full document
13
Near-simultaneous magnetotail flux rope observations with Cluster and Double Star
... and TC-1. Signatures 1 and 2, therefore cannot represent one straight flux ...Signatures 1 and 2 are of different orientations, do not lie along the line separating Cluster and ... See full document
11
Interplanetary shock transmitted into the Earth’s magnetosheath: Cluster and Double Star observations
... following double bow shock crossings when TC1 goes from the magnetosheath to the solar wind at 19:17 UT and then returns back into the magnetosheath 5 min ...by star and cross, ... See full document
16
Simultaneous Double Star and Cluster FTEs observations on the dawnside flank of the magnetosphere
... that reconnection was still occur- ring between the magnetosheath and closed magnetospheric field ...and TC-1 imply that the reconnected flux tubes were moving southward from a common ... See full document
11
First results of low frequency electromagnetic wave detector of TC-2/Double Star program
... reported observations from OGO-5 in which ULF magnetic fluctuations were detected at the polar cusp boundaries and were probably due to the Kevin-Helmholtz ... See full document
9
Radial variation of whistler-mode chorus: first results from the STAFF/DWP instrument on board the Double Star TC-1 spacecraft
... the TC-1 spacecraft are needed to verify these first ...Future observations on the nightside will be especially inter- esting, because of the importance of the nightside storm-time chorus for the ... See full document
6
Characterization of the planetary nebula Tc 1 based on VLT X-shooter observations
... VLT/X-Shooter observations of the planetary nebula Tc ...a double peak spectral profile consistent with the blue- and red-shifted components of an expanding spherical ...that Tc 1 is a ... See full document
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