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chromosphere ne demek?

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İngilizce - Türkçe

chromosphere anlamı
kromosfer

"chromosphere" için örnek kullanımlar

Between the two layers, the chromosphere clocks in at around 4000ºC.

Iki kat, yaklaşık 4000 º C'de yılında kromosfer saatleri arasında

Kaynak: itechpost.com

It targets water as the chromosphere to absorb the laser energy.

Bu lazer enerjisini absorbe kromosfer olarak su hedefliyor.

Kaynak: wftv.com

Even stranger is a curious temperature minimum of 4000 degrees lying between the two layers, in the chromosphere.

Hatta yabancı kromosfer yılında, iki kat arasında uzanan 4000 derece meraklı bir sıcaklığı minimumdur.

Kaynak: redorbit.com

More information: Their paper, titled "Propagation of Alfvénic Waves from Corona to Chromosphere and Consequences for Solar Flares", is published in the Astrophysical Journal.

Daha fazla bilgi: "Corona kromosfer ve Güneş fişekleri için Sorunlarıyla Alfvénic Dalgalarının Yayılması" başlıklı Onların kağıt, Astrophysical Journal dergisinde yayınlandı.

Kaynak: phys.org

The chromosphere (literally, "sphere of color") is the second of the three main layers in the Sun 's atmosphere and is roughly 2,000
Kaynak: Chromosphere

spicules , Hα filaments and plages in the chromosphere, prominences in the chromosphere and transition region, and flares and coronal
Kaynak: Corona

It is called the chromosphere from the Greek root chroma, meaning color, because the chromosphere is visible as a colored flash at the
Kaynak: Sun

In solar physics , a spicule is a dynamic jet of about 500 km diameter in the chromosphere of the Sun . It moves upwards at about 20 km/s
Kaynak: Spicule (solar physics)

Solar flares affect all layers of the solar atmosphere (photosphere , chromosphere , and corona ), when the plasma medium is heated to
Kaynak: Solar flare

A plage is a bright region in the chromosphere of the Sun , typically found in regions of the chromosphere near sunspots . The term
Kaynak: Plage (astronomy)

Plage (astronomy), a bright region in the chromosphere of the Sun. Plage (mycology), a clear, unornamented area on the basal area of an
Kaynak: Plage

plasma , which do not emit much visible light , prominences contain much cooler plasma, similar in composition to that of the chromosphere .
Kaynak: Solar prominence

The solar transition region is a region of the Sun 's atmosphere, between the chromosphere and corona It is visible from space using
Kaynak: Solar transition region

other layers Observed during eclipse, the sun's chromosphere appears (briefly) as a thin pinkish arc and its corona is seen as a tufted halo .
Kaynak: Stellar atmosphere

(chromosphere and corona The term space weather is sometimes used to refer to changes in interplanetary (and occasionally interstellar
Kaynak: Space weather

(traditionally divided into chromosphere , transition region and corona ), and, in particular, the processes of production of the
Kaynak: Coronal radiative losses

The Sun's visible atmosphere has other layers above the photosphere: the 2,000 kilometer-deep chromosphere (typically observed by filtered
Kaynak: Photosphere

Burbank who spotted them in 1959- He discovered them in time-lapse photography of the chromosphere in the light of the Balmer alpha transition .
Kaynak: Moreton wave

Imaging Spectrograph aboard Hubble, the team likened the rise and fall of convection cells in the chromosphere to the blobs in a lava lamp .
Kaynak: Betelgeuse

He discovered the physical properties of the solar chromosphere , the chemistry of stars, the atmosphere of Mars, and the nature of
Kaynak: Donald Howard Menzel

The MLSO is tasked with monitoring the solar atmosphere and recording data on plasmic and energetic emissions from the chromosphere
Kaynak: Mauna Loa Solar Observatory

They are close binary stars having active chromosphere s which can cause large stellar spots. These spots are believed to cause
Kaynak: RS Canum Venaticorum variable

The variability is attributed to large-scale magnetic activity on the chromosphere (in the form of starspot s) combined with a rotational
Kaynak: 12 Ophiuchi

line formed at a temperature below 10 5 K; this fact would imply a constant downflow from the transition region towards the chromosphere .
Kaynak: Evershed effect

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