อภิธานศัพท์ฟิสิกส์ (อวกาศ)
Completion requirements
อภิธานศัพท์ฟิสิกส์ (อวกาศ)
เลือกดูโดยใช้ดัชนีคำศัพท์
พิเศษ | A | B | C | D | E | F | G | H | I | J | K | L | M | N | O | P | Q | R | S | T | U | V | W | X | Y | Z | ก | ข | ค | ฆ | ง | จ | ฉ | ช | ซ | ฌ | ญ | ฎ | ฏ | ฐ | ฑ | ฒ | ณ | ด | ต | ถ | ท | ธ | น | บ | ป | ผ | ฝ | พ | ฟ | ภ | ม | ย | ร | ล | ว | ศ | ษ | ส | ห | ฬ | อ | ฮ | ทั้งหมด
C |
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CARRINGTON LONGITUDE A system of fixed longitudes rotating with the sun.
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CENTIMETER BURST A solar radio burst in the centimeter wavelength range.
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CENTRAL MERIDIAN PASSAGE (CMP) The passage of an ACTIVE REGION or other
feature across the longitude meridian that passes through the
apparent center of the solar DISK.
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CHROMOSPHERE The layer of the solar atmosphere above the PHOTOSPHERE and
beneath the transition region and the CORONA.
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CHROMOSPHERIC EVENTS Some flares are just Chromospheric Events
without Centimetric Bursts or Ionospheric
Effects. (SID) (Class C flare)
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CONJUGATE POINTS Two points on the earth's surface, at opposite ends of a
geomagnetic field line.
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CONTINUUM STORM (CTM) General term for solar noise lasting for hours and
sometimes days.
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COORDINATED UNIVERSAL TIME By international agreement, the local time at
the prime meridian, which passes through Greenwich, England.
Therefore, it is also known as GREENWICH MEAN TIME, or sometimes
simply UNIVERSAL TIME.
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CORONA The outermost layer of the solar atmosphere, characterized by low
densities (1.0E+09/cc) and high temperatures (1,0E+06deg.K).
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CORONAL HOLE An extended region of the CORONA, exceptionally low in density
and associated with unipolar photospheric regions.
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CORONAL RAIN (CRN) Material condensing in the CORONA and appearing to rain
down into the CHROMOSPHERE as observed in H-ALPHA at the solar LIMB
above strong SUNSPOTS.
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CORONAL TRANSIENTS A general term for short-time-scale changes in the
CORONA, but principally used to describe outward-moving PLASMA
clouds.
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COSMIC RAY An extremely energetic (relativistic) charged particle.
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CROCHET A sudden deviation in the sunlit geomagnetic field (H component;
see GEOMAGNETIC ELEMENTS) associated with large solar
FLARE X-ray emission.
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