Search Publications

Use of non-radiation hardened micro-circuits in space — Experience from the cluster digital wave processor
DOI: 10.1016/S0273-1177(03)90282-1 Bibcode: 2003AdSpR..32..417Y

Alleyne, H. St. C.; Yearby, K. H.

The trend for higher performance, lower cost, space instrumentation is leading towards the use commercial or industrial electronic parts, rather than specifically radiation hardened military grade parts. The micro-processor and memory devices used in the Cluster Digital Wave Processor (DWP) are not specifically radiation hardened parts, although t…

2003 Advances in Space Research
Cluster 1
Hot loop oscillations seen by SUMER
DOI: 10.1002/asna.200310119 Bibcode: 2003AN....324..340W

Solanki, S. K.; Curdt, W.; Innes, D. E. +2 more

2003 Astronomische Nachrichten
SOHO 1
Chasing coronaij x-ray emission to the end of the pleiades main sequence … and beyond?
DOI: 10.1016/S0273-1177(03)00310-7 Bibcode: 2003AdSpR..32.1081B

Briggs, K. R.; Pye, J. P.

We have used a 40-ks XMM-Newton observation to examine the X-ray emission of 33 proposed M-type members in. the core of the Pleiades. We reach a limiting X-ray luminosity of LX ≈ × 10 27 erg s -1 in the field centre and detect 17 of 19 members with MIc < 10.5 (where MIc

2003 Advances in Space Research
XMM-Newton 1
A transient event in lines of Ne V, VI and VII
DOI: 10.1051/0004-6361:20021891 Bibcode: 2003A&A...401.1131H

Jordan, C.; Houdebine, E. R.

We report observations of a transition region brightening made with the Coronal Diagnostic Spectrometer onboard the Solar and Heliospheric Observatory. We observed a region of the quiet Sun in 12 spectral lines with temperatures of formation from =~ 3 x 104 K to 1.1 x 106 K. The transient event occured in a network boundary r…

2003 Astronomy and Astrophysics
SOHO 1
Eta Carinae: Bullet Streams and Colliding Wind Shocks
Bibcode: 2003RMxAC..15...59C

Currie, D. G.

Eta Carinae, the most massive and most luminous star in our Galaxy, erupted in 1842 with an energy rivaling a supernova. It ejected approximately two solar masses of material to form an extended bipolar nebula (the homunculus), a variety of massive ``bullets'' (NN and NS knots and the South Bar) and the ``spikes'' (long narrow strings of bullets).…

2003 Revista Mexicana de Astronomia y Astrofisica Conference Series
eHST 1
Far-Ultraviolet light curves of the δ Scuti variable: β Cassiopeiae
DOI: 10.1016/S0273-1177(02)00630-0 Bibcode: 2003AdSpR..31..381D

Cugier, H.; Daszyńska, J.

2003 Advances in Space Research
IUE 1
Cluster magnetic field observations of magnetospheric boundaries
DOI: 10.1029/133GM06 Bibcode: 2003GMS...133...63H

Balogh, A.; Horbury, T. S.; Lucek, E. A. +7 more

Early Cluster magnetic field observations of boundaries and boundary layers in the near-Earth environment are reviewed. By combining data from four spacecraft, typically separated by ∼600 km, the scale, orientation and motion of structures can be deduced. Early results from the magnetic field investigation are reviewed, such as estimates of the or…

2003 Geophysical Monograph Series
Cluster 1
Solar observations from space and from the ground
DOI: 10.1002/asna.200310117 Bibcode: 2003AN....324..334C

Curdt, W.

Recent results from space missions like YOHKOH, SOHO or TRACE as well as ground-based observations clearly indicate that physical processes of most solar phenomena take place on small scales, which are still below the resolution of the instruments employed. There is an urgent need for observations at higher resolution and also for their extension …

2003 Astronomische Nachrichten
SOHO 1
Intercalibration of SUMER and CDS on SOHO. III. SUMER and CDS-GIS
DOI: 10.1364/AO.42.000657 Bibcode: 2003ApOpt..42..657P

Solanki, Sami K.; Schühle, Udo; Pauluhn, Anuschka +2 more

Simultaneous observation of the same solar sources with different instruments is one way to test prelaunch radiometric calibrations and to detect changes in responsivity with time of extreme-ultraviolet instruments in space. Here we present the results of intercalibration of the SUMER (Solar Ultraviolet Measurements of Emitted Radiation) spectrome…

2003 Applied Optics
SOHO 1
Excitation of Solar p-mode Oscillations by Flares
Bibcode: 2003BASI...31..319A

Basu, Sarbani; Antia, H. M.; Ambastha, Ashok

Solar flares release large amounts of energy at different layers of the solar atmosphere. It is, therefore, expected that major flares would be able to excite waves, thereby affecting the p-mode oscillation characteristics. From the analysis of MDI data, we find that power in p-modes appears to increase for some flares, beyond the normal values ex…

2003 Bulletin of the Astronomical Society of India
SOHO 1