「Occultation」の共起表現一覧(1語右で並び替え)
該当件数 : 94件
| During the same 1979 | occultation, a hint of a possible 11 km wide satellite |
| GPS Radio | occultation amounts to an almost instantaneous depictio |
| , the Kepler team searched for the planet's | occultation behind its star, hoping to find the tempera |
| On 29 July 1808 there was an | occultation by Neptune. |
| The last | occultation by a planet took place on 13 May 1971, by J |
| A stellar | occultation by Julia was observed on December 20, 1985. |
| One | occultation by Adria has been reported so far, from Jap |
| One stellar | occultation by Loreley has been observed, on July 20, 2 |
| The only observed stellar | occultation by Felicitas is one from Japan (March 29, 2 |
| An | occultation by Laurentia was observed from Clive, Alber |
| A stellar | occultation by Galatea was observed on September 8, 198 |
| A stellar | occultation by Urda was observed from Japan on July 23, |
| There is one reported stellar | occultation by Protogeneia, on May 28, 2002, from Texas |
| One observed stellar | occultation by Antiope has been reported, on June 11, 1 |
| An | occultation by Athor was observed, on October 15, 2002 |
| The next | occultation by a planet takes place on February 17, 203 |
| The last | occultation by a planet was by Saturn on June 30, 1857, |
| Only one stellar | occultation by Alkeste has been observed, when the aste |
| The last | occultation by Venus took place on 27 December 1852 and |
| Bevis has also observed an | occultation by Venus of Mercury on May 28, 1737, and ob |
| An | occultation diameter of ~170 km was measured from the o |
| It is a suspected | occultation double, with both stars having the same mag |
| This was the only asteroid | occultation event visible to the naked eye during the 2 |
| OCCULT4 visualization of 13 Egeria | occultation event of January 22, 2008 |
| There have been four reported stellar | occultation events by Irene. |
| The Ionospheric | Occultation Experiment (IOX) uses a dual frequency Glob |
| d Sramek made a first radio-interferometric | occultation experiment to test the theory of general re |
| ymer Battery Experiment (PBEX), Ionospheric | Occultation Experiment (IOX), Coherent Electromagnetic |
| astable oscillator (USO) for use in a radio | occultation experiment. |
| Occultation experiments in May and June 1972 allowed sc | |
| This | occultation had been attributed to ring arcs, but when |
| TG-D: Trace Gas Detector (solar | occultation; high spectral resolution across broad spec |
| ze of Tokio is 85 km x 60 km (determined by | occultation in Japan on February 18, 2004). |
| Results from the | occultation indicate a larger than expected diameter of |
| GPS Radio | occultation is a relatively new technique (first applie |
| From studying its light curve during | occultation, it is thought that α Cancri A may itself b |
| riments to probe Venus' atmosphere by radio | occultation, measure the hydrogen Lyman-alpha (hard ult |
| The SAGE instruments use solar | occultation measurement technique to determine chemical |
| Solar | occultation measurement technique measures sunlight thr |
| ty of the Pacific for his variable star and | occultation observations in 1997. |
| ard in 1981 for his variable star and lunar | occultation observations and contributions to artificia |
| was determined from the Beatrician stellar | occultation observed on June 15, 1983. |
| The only observed Lachesean | occultation occurred in 1999 and was recorded in the so |
| A lunar | occultation occurs when the Moon, moving along its orbi |
| (152) Atala | occultation of TYC 6180-01003-1 on 2006 Sept 30th |
| Occultation of 2UCAC 31525121 by (130) Elektra - positi | |
| An | occultation of a star by Thisbe was observed on October |
| In 1998 an | occultation of a star by the asteroid was observed from |
| One | occultation of a star by the asteroid has been observed |
| An | occultation of a star by Maria was observed from Manito |
| Occultation of TYC 5558-01048-1 by (152) Atala on 2006 | |
| Ground track of the March 20, 2014 | occultation of Regulus by 163 Erigone. |
| More frequent, however, is an | occultation of a planet by the Moon. |
| A Hekatean | occultation of a star was observed on July 14, 2003, fr |
| An | occultation of a star by Iduna was observed from Mexico |
| One observation of an | occultation of a star by Vala is from Italy (May 26, 20 |
| The next planetary | occultation of Zavijava will take place on 11 August 20 |
| t of an observational campaign regarding an | occultation of Regulus by Venus. |
| eter of 178 kilometres was measured from an | occultation of a star on December 10, 1995. |
| An | occultation of a star by Minerva was observed in France |
| h 18, 2007 by Bruno Sicardy to view Pluto's | occultation of a star in Sagitarrius. |
| eight years of research, he found the first | occultation of a star by a black hole. |
| The last | occultation of Nunki by a planet took place on November |
| In 1984 an | occultation of a star produced seven chords that Kriste |
| The asteroid was involved in the | occultation of a 10th magnitude star in the constellati |
| Another asteroid | occultation of Io (magnitude 13.2) occurred on March 12 |
| Global Ozone Monitoring by | Occultation of Stars (GOMOS), is an instrument on board |
| The last planetary | occultation of Spica occurred when Venus passed in fron |
| The | occultation of Alhena (γ Geminorum) by Myrrha was obser |
| An | occultation of Bamberga was observed on 8 December 1987 |
| The last | occultation of ξ² Sagittarii by a planet took place on |
| A low probability asteroid | occultation of star UCAC2 17967364 with an apparent mag |
| Due to | occultation of the primary by the dimmer companion, the |
| On 14 July 1715 Pound observed an | occultation of a star by Jupiter, on 30 October an ecli |
| In 1978 his observation of the | occultation of the asteroid 532 Herculina with the star |
| aculate Imams, and in the time of the major | occultation of the 12th Imam, the Islamic Jurist is bes |
| Following anomalous observations during an | occultation of the star SAO 120774 in 1978, Herculina b |
| There was on | occultation on October 31, 2006, and on December 5, 200 |
| An | occultation on March 19, 1981, suggested a diameter of |
| Observations of an | occultation on 11 February 2006, produced only two chor |
| However, since an | occultation only produces a 2D cross-sectional profile |
| The | occultation path crossed central Europe along a band th |
| Occultation phenomena permitted a determination of the | |
| Integrated GPS | Occultation Receiver (IGOR) |
| January 2011 the band was taken on board by | Occultation Records and entered Parr Street studios in |
| As director of the | occultation section of the Royal Astronomical Society o |
| However, a 2004 | occultation showed a cross-sectional profile of only 48 |
| ncipal investigator for the Taiwan American | Occultation Survey, a project aimed at taking a census |
| intervals; might combine nadir, limb and/or | occultation viewing) |
| One Thetidian stellar | occultation was observed from Oregon in 1999. |
| 2008, Egeria occulted another star and this | occultation was timed by several observers in New Mexic |
| A possible | occultation was observed by Oscar Canales Moreno on Oct |
| The first Cybelian stellar | occultation was observed on October 17, 1979 in the Sov |
| The next | occultation will occur on September 2, 2197, when Venus |
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