Search Publications

Helioseismic Studies of Differential Rotation in the Solar Envelope by the Solar Oscillations Investigation Using the Michelson Doppler Imager
DOI: 10.1086/306146 Bibcode: 1998ApJ...505..390S

Kosovichev, A. G.; Hoeksema, J. T.; Scherrer, P. H. +21 more

The splitting of the frequencies of the global resonant acoustic modes of the Sun by large-scale flows and rotation permits study of the variation of angular velocity Ω with both radius and latitude within the turbulent convection zone and the deeper radiative interior. The nearly uninterrupted Doppler imaging observations, provided by the Solar O…

1998 The Astrophysical Journal
SOHO 847
The structure and origin of magnetic clouds in the solar wind
DOI: 10.1007/s00585-997-0001-x Bibcode: 1998AnGeo..16....1B

Schwenn, R.; Bothmer, V.

Plasma and magnetic field data from the Helios 1/2 spacecraft have been used to investigate the structure of magnetic clouds (MCs) in the inner heliosphere. 46 MCs were identified in the Helios data for the period 1974-1981 between 0.3 and 1 AU. 85% of the MCs were associated with fast-forward interplanetary shock waves, supporting the close assoc…

1998 Annales Geophysicae
SOHO 622
SOHO/EIT observations of an Earth-directed coronal mass ejection on May 12, 1997
DOI: 10.1029/98GL50429 Bibcode: 1998GeoRL..25.2465T

St. Cyr, O. C.; Plunkett, S. P.; Michels, D. J. +3 more

An earth-directed coronal mass ejection (CME) was observed on May 12, 1997 by the SOHO Extreme ultraviolet Imaging Telescope (EIT). The CME, originating north of the central solar meridian, was later observed by the Large Angle Spectrometric Coronagraph (LASCO) as a “halo” CME: a bright expanding ring centered about the occulting disk. Beginning a…

1998 Geophysical Research Letters
SOHO 609
UVCS/SOHO Empirical Determinations of Anisotropic Velocity Distributions in the Solar Corona
DOI: 10.1086/311434 Bibcode: 1998ApJ...501L.127K

Romoli, M.; Raymond, J. C.; Naletto, G. +28 more

We present a self-consistent empirical model for several plasma parameters of a polar coronal hole near solar minimum, derived from observations with the Solar and Heliospheric Observatory Ultraviolet Coronagraph Spectrometer. The model describes the radial distribution of density for electrons, H0, and O5+ and the outflow ve…

1998 The Astrophysical Journal
SOHO 434
How uncertain are solar neutrino predictions?
DOI: 10.1016/S0370-2693(98)00657-1 Bibcode: 1998PhLB..433....1B

Basu, Sarbani; Pinsonneault, M. H.; Bahcall, John N.

Solar neutrino fluxes and sound speeds are calculated using a systematic reevaluation of nuclear fusion rates. The largest uncertainties are identified and their effects on the solar neutrino fluxes are estimated.

1998 Physics Letters B
SOHO 382
The Sun's total irradiance: Cycles, trends and related climate change uncertainties since 1976
DOI: 10.1029/1998GL900157 Bibcode: 1998GeoRL..25.4377F

Fröhlich, Claus; Lean, Judith

A composite record of the Sun's total irradiance compiled from measurements made by five independent space-based radiometers since 1978 exhibits a prominent 11-year cycle with similar levels during 1986 and 1996, the two most recent minimum epochs of solar activity. This finding contradicts recent assertions of a 0.04% irradiance increase from the…

1998 Geophysical Research Letters
SOHO 359
The Solar Corona Above Polar Coronal Holes as Seen by SUMER on SOHO
DOI: 10.1086/305756 Bibcode: 1998ApJ...500.1023W

Wilhelm, Klaus; Marsch, Eckart; Dwivedi, Bhola N. +4 more

In order to address two of the principal scientific objectives of the Solar and Heliospheric Observatory (SOHO), studies of the heating mechanisms of the solar corona and the acceleration processes of the solar wind, we deduce electron temperatures, densities, and ion velocities in plumes and interplume regions of polar coronal holes using ultravi…

1998 The Astrophysical Journal
SOHO 274
Energy Distribution of Heating Processes in the Quiet Solar Corona
DOI: 10.1086/311474 Bibcode: 1998ApJ...501L.213K

Krucker, Säm; Benz, Arnold O.

We have determined the variations in the emission measure of the solar corona using EUV Imaging Telescope/Solar and Heliospheric Observatory observations of iron lines in a quiet region of the Sun. The emission measure is found to vary significantly in at least 85% of all the pixels within 42 minutes. The variations are interpreted as heating even…

1998 The Astrophysical Journal
SOHO 243
X-ray flare sparks quake inside Sun
DOI: 10.1038/30629 Bibcode: 1998Natur.393..317K

Kosovichev, A. G.; Zharkova, V. V.

Solar flares involve a release of the Sun's magnetic energy as X-radiation, particle beams and high-speed plasma flows. But we have discovered, using data from the Solar and Heliospheric Observatory (SOHO), that these flares also affect the Sun's interior, generating seismic waves similar to earthquakes. For example, a three-kilometre-high seismic…

1998 Nature
SOHO 217
SUMER Measurements of Nonthermal Motions: Constraints on Coronal Heating Mechanisms
DOI: 10.1086/306179 Bibcode: 1998ApJ...505..957C

Chae, Jongchul; Schühle, Udo; Lemaire, Philippe

We have determined nonthermal velocities in the quiet Sun at temperatures between 104 K and 2 × 106 K by measuring the widths of a number of EUV and far-ultraviolet (FUV) lines taken with SUMER on board the SOHO spacecraft. The broadenings owing to the SUMER instrument and the finite opacity in each line have been carefully e…

1998 The Astrophysical Journal
SOHO 196