ملف:1998 OR2 Radar.gif

مافيش ريزوليوشن اعلى متوفر.

1998_OR2_Radar.gif (400 × 400 بكسل حجم الفايل: 1.08 ميجابايت، نوع MIME: image/gif، ملفوف، 10 براويز، 1.5ث)

الملف دا من ويكيميديا كومنز و ممكن تستعمله المشاريع التانيه. الوصف بتاعه صفحة وصف الملف هناك معروض تحت..

الخلاصة

وصف1998 OR2 Radar.gif	English: Animation of delay-Doppler images from Apr 18 UT.
تاريخ	18 ابريل 2020
مصدر	http://www.naic.edu/~pradar/press/1998OR2.php
مؤلف	Arecibo Observatory/NASA/NSF

الترخيص

	يقع هذا العمل في النِّطاق العامّ في الولايات المُتحدة الأمريكيَّة لأَنَّه عملٌ خالِصٌ من إِنتاج وكالة الفضاء الأمريكيَّة. تنصُ حقوق التَّأليف والنَّشر الخاصَّة بوكالة الفضاء الأمريكيَّة على أنَّ "أعمال الوكالة غير مَحميَّة بحقوق التَّأليف والنَّشر ما لم يُذكر خلافُ ذلك". لمزيدٍ من المعلومات انظر القالِب {{PD-USGov}} وصفحة حقوق التَّأليف والنَّشر الخاصَّة بالوكالة وصفحة سياسة الصُّور الخاصَّة بمُختبر الدَّفع النَّفَّاث.
	تنبيهات: إنَّ استعمال شعار الوكالة، وشاراتها ولافتاتها مُقيَّدٌ بالقانون الأَمريكيّ 14 CFR 1221. يستضيف موقع الوكالة عدداً كبيراً من الصُّور من إِنتاج برنامج الفضاء السُّوفيتي أو وكالة الفضاء الاتحاديَّة الرُّوسيَّة ووكالات فضاء أخرى غير أمريكيَّة، ولا يجب الافتراض أن هذه الصُّور تقع في النِّطاق العامّ. إنَّ المواد المُنتَجة اعتماداً على بيانات مَرصد هابِل الفضائيّ قد تكون مَحميَّةً بحقوق التَّأليف والنَّشر ما تكن مُنتَجةً صراحةً بواسطة معهد مراصِد علوم الفضاء. انظر صفحة حقوق التَّأليف والنَّشر الخاصَّة بالمرصد وأيضاً القالبين {{PD-Hubble}} و{{Cc-Hubble}}. إنَّ جميع المواد المُنشأة بواسطة مُستشعِرات مِسبار الشمس وغلافها محميَّة بحقوق التَّأليف والنَّشر، ويلزم الحصول على تصريح قبل استعمالها في الأنشطة غير الرِّبحيَّة. انظر صفحة حقوق التَّأليف والنَّشر الخاصَّة بالمِسبار. الصُّور المَنشُورة على موقع صُورة اليوم الفلكيَّة قد تكون مَحميَّةً بحقوق التَّأليف والنَّشر. تشير photo gallery صفحة الأَسئِلة المُتكرِرة لمَجمُوعة الصُّور إلى أنَّ الصُّور المَوجُودة في المَجمُوعة تقع في النِّطاق العامّ ما لم يُذكر خلاف ذلك.

تاريخ الفايل

اضغط على الساعه/التاريخ علشان تشوف الفايل زى ما كان فى الوقت ده.

	الساعه / التاريخ	صورة صغيرة	ابعاد	يوزر	تعليق
دلوقتي	17:26، 23 ابريل 2020		400 × 400 (1.08 ميجابايت)	Nrco0e	Uploaded a work by Arecibo Observatory/NASA/NSF from http://www.naic.edu/~pradar/press/1998OR2.php with UploadWizard

استخدام الفايل

ال1 صفحة دى فيها وصله للفايل ده:

(52768) 1998 OR2 (كويكب)

استخدام الملف العام

الويكيات التانيه دى بتستخدم الفايل ده:

الاستخدام ف ar.wikipedia.org
- (52768) 1998 OR2
الاستخدام ف be.wikipedia.org
- (52768) 1998 OR2
الاستخدام ف en.wikipedia.org
- (52768) 1998 OR2
- List of asteroid close approaches to Earth in 2020
الاستخدام ف eo.wikipedia.org
- (52768) 1998 OR2
الاستخدام ف eu.wikipedia.org
- (52768) 1998 OR2
الاستخدام ف fi.wikipedia.org
- (52768) 1998 OR2
الاستخدام ف hr.wikipedia.org
- (52768) 1998 OR2
الاستخدام ف ja.wikipedia.org
- (52768) 1998 OR2
الاستخدام ف pl.wikipedia.org
- (52768) 1998 OR2
الاستخدام ف ru.wikipedia.org
- (52768) 1998 OR2
الاستخدام ف sv.wikipedia.org
- 1998 OR2
الاستخدام ف uz.wikipedia.org
- Asteroid OR2 1998
الاستخدام ف vi.wikipedia.org
- (52768) 1998 OR2
الاستخدام ف www.wikidata.org
- Q8331812

بيانات ميتا

الملف ده فيه معلومات إضافيه، غالبا ما تكون أضيفت من الديجيتال كاميرا أو السكانر ح الضوئى المستخدم فى نقل الملف للكومبيوتر.

إذا كان الملف اتعدل عن حالته الأصلية، فبعض التفاصيل مش ها تعبر عن الملف المعدل.

تعليق ملف GIF

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 Additional -6.45466400328587e-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 Additional -1.82322992259287e-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 Additional -6.50443183758398e-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 Additional -1.81660055886823e-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 Additional -3.99515300841813e-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 Additional -8.91766944732808e-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 Additional -9.82426371365364e-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 Additional -8.59829185628769e-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 Additional -5.33652837475529e-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 Additional 0 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.

ملف:1998 OR2 Radar.gif

الخلاصة

الترخيص

الشروحات

العناصر المصورة في هذا الملف

يُصوِّر ^{العربية}

(52768) 1998 OR2 (كويكب)

حالة حقوق التأليف والنشر ^{العربية}

ملكيه عامه

البدايه

18 ابريل 2020

نوع الوسائط ^{العربية}

image/gif

تدقيق المجموع ^{العربية}

9d1afd27a456ca9a88cd538f75ce6e3c02064534

حجم البيانات ^{العربية}

1,134,988 بايت

المدة ^{العربية}

1.5 ثانيه

الارتفاع ^{العربية}

400 بكسل

العرض

400 بكسل

تاريخ الفايل

استخدام الفايل

استخدام الملف العام

بيانات ميتا

ملف:1998 OR2 Radar.gif

الخلاصة

الترخيص

الشروحات

العناصر المصورة في هذا الملف

يُصوِّر العربية

(52768) 1998 OR2 (كويكب)

حالة حقوق التأليف والنشر العربية

ملكيه عامه

البدايه

18 ابريل 2020

نوع الوسائط العربية

image/gif

تدقيق المجموع العربية

9d1afd27a456ca9a88cd538f75ce6e3c02064534

حجم البيانات العربية

1,134,988 بايت

المدة العربية

1.5 ثانيه

الارتفاع العربية

400 بكسل

العرض

400 بكسل

تاريخ الفايل

استخدام الفايل

استخدام الملف العام

بيانات ميتا

يُصوِّر ^{العربية}

حالة حقوق التأليف والنشر ^{العربية}

نوع الوسائط ^{العربية}

تدقيق المجموع ^{العربية}

حجم البيانات ^{العربية}

المدة ^{العربية}

الارتفاع ^{العربية}