SOHO EIT Carrington maps from synoptic full-disk data

B. J. Thompson; J. S. Newmark; J. B. Gurman; J. P. Delaboudiniere; F. Clette; S. E. Gibson

SOHO EIT Carrington maps from synoptic full-disk data

B. J. Thompson, J. S. Newmark, J. B. Gurman, J. P. Delaboudiniere, F. Clette, S. E. Gibson

HAO Administrative Office

Research output: Contribution to journal › Article › peer-review

4 Scopus citations

Abstract

Since May 1996, the SOHO/EIT daily synoptic observing plan has included at least one full-resolution full-disk image in each EIT bandpass: 171 Å (Fe IX/X), 195 Å (Fe XII), 284 Å (Fe XV) and 304 Å (He II/Si XI). Beginning July 1996, the nominal synoptic sequence has included several sets of half-resolution images in addition to the full-resolution images. These synoptic data sets are combined to make synoptic maps beginning at Carrington Rotation 1911. The synoptic maps at the solar meridian are generated in all four EIT wavelengths, using the same formalism as Yohkoh Soft X-ray Telescope synoptic maps. The off-limb maps at 1.05 and 1.10 solar radii are generated for the three coronal lines using the standard applied to coronagraph synoptic maps.

Original language	English
Pages (from-to)	779-783
Number of pages	5
Journal	European Space Agency, (Special Publication) ESA SP
Issue number	404
State	Published - 1997

Keywords

Coronal Structure

Cite this

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title = "SOHO EIT Carrington maps from synoptic full-disk data",

abstract = "Since May 1996, the SOHO/EIT daily synoptic observing plan has included at least one full-resolution full-disk image in each EIT bandpass: 171 {\AA} (Fe IX/X), 195 {\AA} (Fe XII), 284 {\AA} (Fe XV) and 304 {\AA} (He II/Si XI). Beginning July 1996, the nominal synoptic sequence has included several sets of half-resolution images in addition to the full-resolution images. These synoptic data sets are combined to make synoptic maps beginning at Carrington Rotation 1911. The synoptic maps at the solar meridian are generated in all four EIT wavelengths, using the same formalism as Yohkoh Soft X-ray Telescope synoptic maps. The off-limb maps at 1.05 and 1.10 solar radii are generated for the three coronal lines using the standard applied to coronagraph synoptic maps.",

keywords = "Coronal Structure",

author = "Thompson, \{B. J.\} and Newmark, \{J. S.\} and Gurman, \{J. B.\} and Delaboudiniere, \{J. P.\} and F. Clette and Gibson, \{S. E.\}",

year = "1997",

language = "English",

pages = "779--783",

journal = "European Space Agency, (Special Publication) ESA SP",

issn = "0379-6566",

publisher = "European Space Agency",

number = "404",

}

TY - JOUR

T1 - SOHO EIT Carrington maps from synoptic full-disk data

AU - Thompson, B. J.

AU - Newmark, J. S.

AU - Gurman, J. B.

AU - Delaboudiniere, J. P.

AU - Clette, F.

AU - Gibson, S. E.

PY - 1997

Y1 - 1997

N2 - Since May 1996, the SOHO/EIT daily synoptic observing plan has included at least one full-resolution full-disk image in each EIT bandpass: 171 Å (Fe IX/X), 195 Å (Fe XII), 284 Å (Fe XV) and 304 Å (He II/Si XI). Beginning July 1996, the nominal synoptic sequence has included several sets of half-resolution images in addition to the full-resolution images. These synoptic data sets are combined to make synoptic maps beginning at Carrington Rotation 1911. The synoptic maps at the solar meridian are generated in all four EIT wavelengths, using the same formalism as Yohkoh Soft X-ray Telescope synoptic maps. The off-limb maps at 1.05 and 1.10 solar radii are generated for the three coronal lines using the standard applied to coronagraph synoptic maps.

AB - Since May 1996, the SOHO/EIT daily synoptic observing plan has included at least one full-resolution full-disk image in each EIT bandpass: 171 Å (Fe IX/X), 195 Å (Fe XII), 284 Å (Fe XV) and 304 Å (He II/Si XI). Beginning July 1996, the nominal synoptic sequence has included several sets of half-resolution images in addition to the full-resolution images. These synoptic data sets are combined to make synoptic maps beginning at Carrington Rotation 1911. The synoptic maps at the solar meridian are generated in all four EIT wavelengths, using the same formalism as Yohkoh Soft X-ray Telescope synoptic maps. The off-limb maps at 1.05 and 1.10 solar radii are generated for the three coronal lines using the standard applied to coronagraph synoptic maps.

KW - Coronal Structure

UR - https://www.scopus.com/pages/publications/5544306607

M3 - Article

AN - SCOPUS:5544306607

SN - 0379-6566

SP - 779

EP - 783

JO - European Space Agency, (Special Publication) ESA SP

JF - European Space Agency, (Special Publication) ESA SP

IS - 404

ER -

SOHO EIT Carrington maps from synoptic full-disk data

Abstract

Keywords

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