Browse terms - alphabetical

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Term Definition Contributor Modified
Brunogeierite No definition provided Ryan McGranaghan 2023.04.16
Brunsvigite No definition provided Ryan McGranaghan 2023.04.16
brunt vaisala frequency The frequency at which a displaced parcel will oscillate when displaced vertically within a statically stable environment. Ryan McGranaghan 2023.04.16
Brush arc-light system No definition provided Christopher Rauch 2023.12.01
Brushes No definition provided Christopher Rauch 2023.12.01
Brushes, Carbon No definition provided Christopher Rauch 2023.12.01
Brushite No definition provided Ryan McGranaghan 2023.04.16
Brush-Swan electric light system No definition provided Christopher Rauch 2023.12.01
Brutes No definition provided Christopher Rauch 2023.12.01
Bryology No definition provided Christopher Rauch 2023.12.01
Bryophytes No definition provided Christopher Rauch 2023.12.01
Bryozoa No definition provided Christopher Rauch 2023.12.01
bs The BS climate classification, also known as semiarid climate classification, is characterized by having precipitation amounts greater than 1/2 potential evapotranspiration (POTET), but not equal to i t. Ryan McGranaghan 2023.04.16
bsh The BSh climate classification, also known as the hot low-latitude steppe, is characterized by having mean annual temperatures greater than 18 degree C. Ryan McGranaghan 2023.04.16
bsk The BSk climate classification, also known as cold midlatitude steppe climate classification, is characterized by having mean annual temperatures less than 18 degree C. Ryan McGranaghan 2023.04.16
b spline No definition provided Ryan McGranaghan 2023.04.16
B stars A star of spectral type B, whose spectrum is marked by absorption lines of hydrogen; also known as B-type star. B-type optical spectra are characterized by the presence of neutral He lines (mainly He I 4471 Å) at about type B9. He I strengthens up to about B2, then decreases. Ionized helium (mainly He II 4541 Å) first appears at about B0. Most metallic lines are absent or weak, except some absorption lines for the higher ionization states of silicon, oxygen, carbon, and magnesium. These are hot stars with effective temperatures ranging from about 10,000 K at B9 to nearly 30,000 K at B0. They are between 3 and 20 solar masses. Some famous examples include Rigel, Achernar, and Hadar. Ryan McGranaghan 2023.04.16
B stars A star of spectral type B, whose spectrum is marked by absorption lines of hydrogen; also known as B-type star. B-type optical spectra are characterized by the presence of neutral He lines (mainly He I 4471 Å) at about type B9. He I strengthens up to about B2, then decreases. Ionized helium (mainly He II 4541 Å) first appears at about B0. Most metallic lines are absent or weak, except some absorption lines for the higher ionization states of silicon, oxygen, carbon, and magnesium. These are hot stars with effective temperatures ranging from about 10,000 K at B9 to nearly 30,000 K at B0. They are between 3 and 20 solar masses. Some famous examples include Rigel, Achernar, and Hadar. Ryan McGranaghan 2023.04.16
B subdwarf stars No definition provided Ryan McGranaghan 2023.04.16
B subdwarf stars No definition provided Ryan McGranaghan 2023.04.16
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