Fichier:Atira.20jan17.u2.s1p0.gif

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Atira.20jan17.u2.s1p0.gif ‎(200 × 170 Pixel, Fichiersgréisst: 204 KB, MIME-Typ: image/gif, endlos Schleef, 9 Biller, 0,9 s)

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Resumé

BeschreiwungAtira.20jan17.u2.s1p0.gif	English: Radar images of 163693 Atira, taken at Arecibo Observatory on 20 January 2017
Datum	29. Mee 2017
Quell	http://outreach.naic.edu/ao/blog/discovery-announcement-binary-system-163693-atira
Auteur	Arecibo Observatory, NASA

Lizenz

	Diese Datei ist gemeinfrei (public domain), da sie von der NASA erstellt worden ist. Die NASA-Urheberrechtsrichtlinie besagt, dass „NASA-Material nicht durch Urheberrecht geschützt ist, wenn es nicht anders angegeben ist“. (NASA-Urheberrechtsrichtlinie-Seite oder JPL Image Use Policy).
	Warnung: Die Verwendung von NASA-Logos, Wappen und Symbolen ist durch das US-Gesetz 14 CFR 1221 eingeschränkt. Die NASA-Homepage hostet viele Bilder der Sowjetischen bzw. Russischen Raumfahrtagentur sowie anderer nicht-amerikanischer Raumfahrtagenturen. Diese sind nicht gemeinfrei. Material des Hubble-Weltraumteleskops kann urheberrechtlich geschützt sein, wenn es nicht ausdrücklich vom STScI ist. [1] Jegliches Material des Solar and Heliospheric Observatory (SOHO) ist urheberrechtlich geschützt und benötigt eine gesonderte Genehmigung für kommerzielle, nicht-pädagogische Zwecke. [2] Bilder, die als Astronomie-Bild des Tages (APOD) veröffentlicht werden, sind unter Umständen urheberrechtlich geschützt. [3]

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Benotzt op ar.wikipedia.org
- أتيرا (163693)
Benotzt op arz.wikipedia.org
- (163693) Atira (كويكب)
Benotzt op ca.wikipedia.org
- (163693) Atira
Benotzt op en.wikipedia.org
- List of Solar System objects by size
- 163693 Atira
Benotzt op es.wikipedia.org
- (163693) Atira
Benotzt op fr.wikipedia.org
- (163693) Atira
Benotzt op it.wikipedia.org
- 163693 Atira
Benotzt op mk.wikipedia.org
- Список на тела во Сончевиот Систем по големина
Benotzt op nl.wikipedia.org
- 163693 Atira
Benotzt op pl.wikipedia.org
- (163693) Atira
Benotzt op ru.wikipedia.org
- (163693) Атира
Benotzt op sk.wikipedia.org
- 163693 Atira
Benotzt op sv.wikipedia.org
- 163693 Atira
Benotzt op www.wikidata.org
- Q141774

Metadaten

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Bemierkung zum GIF-Fichier

FITS (Flexible Image Transport System) format is defined in 'Astronomy and Astrophysics', volume 376, page 359; bibcode: 2001A&A...376..359H The RX start time is a reasonable approximation to the experiment mid-time. A more accurate mid-time is DATE-OBS + (EXPTIME-RTT)/2 which is typically about 3s earlier Frequency axis reversed in writefits. Additional -5.00609758091741e-08 s added: Range curvature correction If FREQSAMP < FFTLEN, then the transform was zero-filled SAMPPBD is the number of input samples taken per baud. ROWSPBD is the number of output image rows saved per baud. ROWSPBD and SAMPPBD may differ either because data were thrown away, or because the extra samples were used in the frequency processing. CODEPROC is the code processing method: values are short, long_orig, or long_mod. short means short-code data processed so that each Doppler fft includes data from all samples per baud; long_mod means long-code data processed in the same way; long_orig means long-code data where each sample per baud is processed separately and the separate images are then interleaved in delay.
FITS (Flexible Image Transport System) format is defined in 'Astronomy and Astrophysics', volume 376, page 359; bibcode: 2001A&A...376..359H The RX start time is a reasonable approximation to the experiment mid-time. A more accurate mid-time is DATE-OBS + (EXPTIME-RTT)/2 which is typically about 3s earlier Frequency axis reversed in writefits. Additional -2.30660930355953e-08 s added: Range curvature correction If FREQSAMP < FFTLEN, then the transform was zero-filled SAMPPBD is the number of input samples taken per baud. ROWSPBD is the number of output image rows saved per baud. ROWSPBD and SAMPPBD may differ either because data were thrown away, or because the extra samples were used in the frequency processing. CODEPROC is the code processing method: values are short, long_orig, or long_mod. short means short-code data processed so that each Doppler fft includes data from all samples per baud; long_mod means long-code data processed in the same way; long_orig means long-code data where each sample per baud is processed separately and the separate images are then interleaved in delay.
FITS (Flexible Image Transport System) format is defined in 'Astronomy and Astrophysics', volume 376, page 359; bibcode: 2001A&A...376..359H The RX start time is a reasonable approximation to the experiment mid-time. A more accurate mid-time is DATE-OBS + (EXPTIME-RTT)/2 which is typically about 3s earlier Frequency axis reversed in writefits. Additional -1.20704157779983e-07 s added: Range curvature correction If FREQSAMP < FFTLEN, then the transform was zero-filled SAMPPBD is the number of input samples taken per baud. ROWSPBD is the number of output image rows saved per baud. ROWSPBD and SAMPPBD may differ either because data were thrown away, or because the extra samples were used in the frequency processing. CODEPROC is the code processing method: values are short, long_orig, or long_mod. short means short-code data processed so that each Doppler fft includes data from all samples per baud; long_mod means long-code data processed in the same way; long_orig means long-code data where each sample per baud is processed separately and the separate images are then interleaved in delay.
FITS (Flexible Image Transport System) format is defined in 'Astronomy and Astrophysics', volume 376, page 359; bibcode: 2001A&A...376..359H The RX start time is a reasonable approximation to the experiment mid-time. A more accurate mid-time is DATE-OBS + (EXPTIME-RTT)/2 which is typically about 3s earlier Frequency axis reversed in writefits. Additional -1.20390581059837e-07 s added: Range curvature correction If FREQSAMP < FFTLEN, then the transform was zero-filled SAMPPBD is the number of input samples taken per baud. ROWSPBD is the number of output image rows saved per baud. ROWSPBD and SAMPPBD may differ either because data were thrown away, or because the extra samples were used in the frequency processing. CODEPROC is the code processing method: values are short, long_orig, or long_mod. short means short-code data processed so that each Doppler fft includes data from all samples per baud; long_mod means long-code data processed in the same way; long_orig means long-code data where each sample per baud is processed separately and the separate images are then interleaved in delay.
FITS (Flexible Image Transport System) format is defined in 'Astronomy and Astrophysics', volume 376, page 359; bibcode: 2001A&A...376..359H The RX start time is a reasonable approximation to the experiment mid-time. A more accurate mid-time is DATE-OBS + (EXPTIME-RTT)/2 which is typically about 3s earlier Frequency axis reversed in writefits. Additional -9.75298348748765e-08 s added: Range curvature correction If FREQSAMP < FFTLEN, then the transform was zero-filled SAMPPBD is the number of input samples taken per baud. ROWSPBD is the number of output image rows saved per baud. ROWSPBD and SAMPPBD may differ either because data were thrown away, or because the extra samples were used in the frequency processing. CODEPROC is the code processing method: values are short, long_orig, or long_mod. short means short-code data processed so that each Doppler fft includes data from all samples per baud; long_mod means long-code data processed in the same way; long_orig means long-code data where each sample per baud is processed separately and the separate images are then interleaved in delay.
FITS (Flexible Image Transport System) format is defined in 'Astronomy and Astrophysics', volume 376, page 359; bibcode: 2001A&A...376..359H The RX start time is a reasonable approximation to the experiment mid-time. A more accurate mid-time is DATE-OBS + (EXPTIME-RTT)/2 which is typically about 3s earlier Frequency axis reversed in writefits. Additional -1.15528564492706e-07 s added: Range curvature correction If FREQSAMP < FFTLEN, then the transform was zero-filled SAMPPBD is the number of input samples taken per baud. ROWSPBD is the number of output image rows saved per baud. ROWSPBD and SAMPPBD may differ either because data were thrown away, or because the extra samples were used in the frequency processing. CODEPROC is the code processing method: values are short, long_orig, or long_mod. short means short-code data processed so that each Doppler fft includes data from all samples per baud; long_mod means long-code data processed in the same way; long_orig means long-code data where each sample per baud is processed separately and the separate images are then interleaved in delay.
FITS (Flexible Image Transport System) format is defined in 'Astronomy and Astrophysics', volume 376, page 359; bibcode: 2001A&A...376..359H The RX start time is a reasonable approximation to the experiment mid-time. A more accurate mid-time is DATE-OBS + (EXPTIME-RTT)/2 which is typically about 3s earlier Frequency axis reversed in writefits. Additional -1.18025354822748e-07 s added: Range curvature correction If FREQSAMP < FFTLEN, then the transform was zero-filled SAMPPBD is the number of input samples taken per baud. ROWSPBD is the number of output image rows saved per baud. ROWSPBD and SAMPPBD may differ either because data were thrown away, or because the extra samples were used in the frequency processing. CODEPROC is the code processing method: values are short, long_orig, or long_mod. short means short-code data processed so that each Doppler fft includes data from all samples per baud; long_mod means long-code data processed in the same way; long_orig means long-code data where each sample per baud is processed separately and the separate images are then interleaved in delay.
FITS (Flexible Image Transport System) format is defined in 'Astronomy and Astrophysics', volume 376, page 359; bibcode: 2001A&A...376..359H The RX start time is a reasonable approximation to the experiment mid-time. A more accurate mid-time is DATE-OBS + (EXPTIME-RTT)/2 which is typically about 3s earlier Frequency axis reversed in writefits. Additional -1.16263237259773e-07 s added: Range curvature correction If FREQSAMP < FFTLEN, then the transform was zero-filled SAMPPBD is the number of input samples taken per baud. ROWSPBD is the number of output image rows saved per baud. ROWSPBD and SAMPPBD may differ either because data were thrown away, or because the extra samples were used in the frequency processing. CODEPROC is the code processing method: values are short, long_orig, or long_mod. short means short-code data processed so that each Doppler fft includes data from all samples per baud; long_mod means long-code data processed in the same way; long_orig means long-code data where each sample per baud is processed separately and the separate images are then interleaved in delay.
FITS (Flexible Image Transport System) format is defined in 'Astronomy and Astrophysics', volume 376, page 359; bibcode: 2001A&A...376..359H The RX start time is a reasonable approximation to the experiment mid-time. A more accurate mid-time is DATE-OBS + (EXPTIME-RTT)/2 which is typically about 3s earlier Frequency axis reversed in writefits. Additional -1.10070374148563e-07 s added: Range curvature correction If FREQSAMP < FFTLEN, then the transform was zero-filled SAMPPBD is the number of input samples taken per baud. ROWSPBD is the number of output image rows saved per baud. ROWSPBD and SAMPPBD may differ either because data were thrown away, or because the extra samples were used in the frequency processing. CODEPROC is the code processing method: values are short, long_orig, or long_mod. short means short-code data processed so that each Doppler fft includes data from all samples per baud; long_mod means long-code data processed in the same way; long_orig means long-code data where each sample per baud is processed separately and the separate images are then interleaved in delay.

Fichier:Atira.20jan17.u2.s1p0.gif

Resumé

Lizenz

Beschreiwungen

In dieser Datei abgebildete Objekte

Motiv

Grënnungsdatum / Baudatum

29. Mee 2017

MIME-Typ ^Däitsch

image/gif

Prüfsumme ^Däitsch

ef147cf48ffc12580977aed4afaa959634be0000

Dateigröße ^Däitsch

209.139 Byte

Dauer

0,8999999999999999 sec.

Héicht

170 Pixel

Breet

200 Pixel

Versiounen

Benotze vu Fichieren

Globaalt Benotze vum Fichier

Metadaten

Fichier:Atira.20jan17.u2.s1p0.gif

Resumé

Lizenz

Beschreiwungen

In dieser Datei abgebildete Objekte

Motiv

Grënnungsdatum / Baudatum

29. Mee 2017

MIME-Typ Däitsch

image/gif

Prüfsumme Däitsch

ef147cf48ffc12580977aed4afaa959634be0000

Dateigröße Däitsch

209.139 Byte

Dauer

0,8999999999999999 sec.

Héicht

170 Pixel

Breet

200 Pixel

Versiounen

Benotze vu Fichieren

Globaalt Benotze vum Fichier

Metadaten

Grënnungsdatum / Baudatum

MIME-Typ ^Däitsch

Prüfsumme ^Däitsch

Dateigröße ^Däitsch