SPS 101 Flashcards
The Kárman line is how many kilometers/miles above the earths surface?
100 km/62 miles
USSPACECOM domain is how many kilometers/miles above mean sea level?
100 km/62 miles
Exobase is how many kilometers/miles above the Earth surface?
500 to 1000 km/310–620 miles
When it comes to the space demarcation, what are the three standards that we can go by?
International standard, US government, standard, scientific community standard
Defined the Kárman line
The Kárman line is the international standard measuring 100 km/62 miles above the Earth surface.
Define USSPACECOM domain
The USSPACECOM Domain is the US government standard measuring at 100 km/62 miles above mean sea level.
Define Exobase
EXO base is the scientific community standard measuring at 500 to 1000 km/310–620 miles above the earths surface
Define demarcation of space
These measurements/boundaries define where space begins.
The sun is composed of what?
74.9 hydrogen, 23.8% helium, and 1.3 miscellaneous gases.
The sun creates energy through what process?
Nuclear fusion
Name the six main layers of the sun
The core, the radiative zone, the tachocline, the convective zone, the photosphere, the atmosphere.
Defined the core of the sun.
Rotates like a solid and is where fusion occurs.
Define the radiative zone.
Rotates like a fluid and radiates energy.
Define the tachocline.
Generates magnetic field lines and stores magnetic flux. Resides between the convective and radiative layers.
Defined the convective zone.
Rotates like a fluid and transfers heat through convection.
Defined the photosphere.
Also known as the surface and is responsible for 99% of solar radiation.
Define atmosphere.
The atmosphere has four sublayers, all of which are only visible during an eclipse.
The core (description)
0.25 of the sun’s radius.
Fusion occurs
Solid core
Rotates like a solid
radiative zone (description)
Radiates energy through the process of photon, emission and captured by the hydrogen and helium ions.
Moves like a fluid.
Convective zone (description)
uses thermal convection (it boils).
Moving plasma, disrupts magnetic field .
Moves like a fluid
Photosphere (description)
Solar surface – this region of the sun is a opaque (optically dark) to life.
99% of solar radiation
Light from the sun submitted through the interaction of electrons with hydrogen atoms.
Where we can see sunspots
Atmosphere (description)
The solar atmosphere is comprised of several sublayers; chromosphere, transition region, Corona, and heliosphere.
(it’s in the outer layers of the suns energy, which has bubbled up from the interior layers is detected as)
These layers are only viewable during an eclipse .
Solar minimum
Is referred to as the quiet sun.
Few to zero, sunspots, dimmer, EUV and x-rays, in frequent flaring/CME.
Solar maximum
Is referred to as active sun.
Many sunspots, brighter, EUV, and x-rays, and frequent flaring/CME.
Magnetism week or during maximum.