Orig. Qs. Flashcards

(45 cards)

1
Q

In a closed-loop control system the actuators receive commands from the sensors: True or False?

A

False

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2
Q

Identify one example of a disturbance torque that acts to gradually degrade a spacecraft’s attitude.

A

Gravity gradient torque

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3
Q

The angular momentum of a spacecraft is always conserved: True or False?

A

False

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4
Q

Identify the process that combines message data with the carrier frequency before radiowave transmission.

A

Modulation

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5
Q

Identify the antenna performance parameter that specifies how much energy from the transmitter is radiated.

A

Gain

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6
Q

Identify the device inside a radioisotope generator that converts heat into electrical power.

A

Thermocouple or Radioisotope Generators

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7
Q

Identify the thermal actuator that provides a modified form of heat convection on a spacecraft.

A

Heat pipe

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8
Q

Identify one disadvantage of using composite materials for construction of a spacecraft structure.

A

Delamination

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9
Q

Identify the name given to the slope of the stress versus strain curve for a material.

A

Young‚ modulus

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10
Q

Explain the difference between passive and active actuators. Provide an example of each.

A

Passive actuators operate without feedback (e.g., magnets); active actuators use feedback control (e.g., reaction wheels).

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11
Q

Explain why a spacecraft may contain multiple GPS receivers, instead of just one. What is their purpose?

A

To increase redundancy and improve position accuracy in 3D space.

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12
Q

Define antenna gain. What is it referenced to? What are its two components?

A

Gain measures how effectively an antenna directs energy, referenced to isotropic radiator; consists of directivity and efficiency.

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13
Q

Explain the physics & math of gravity-gradient stabilization. When is it used? Why? What is the equation?

A

Used in low Earth orbit to stabilize attitude using Earth’s gravity; Earth’s pull rotates the satelitle into alignment, torque = (3 mu / 2r^3) (l_max-l_min) (sin(2theta))

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14
Q

Explain the physics & math of vibrational resonance. When is it a problem? Why? How can it be avoided?

A

Occurs when excitation frequency matches natural frequency; causes large oscillations; avoided via damping or stiffening.

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15
Q

Explain the physics & math of thermal conduction & radiation. How do they work? What are the equations?

A

Conduction: Q = kAΔT/L,
Radiation: Q = σεAT⁴

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16
Q

Mission constraints are external factors that are not controllable and simply must be met: True or False?

A

True

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17
Q

Identify the dominant form of pressure inside a low beta plasma.

A

Magnetic pressure

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18
Q

Identify the region of the solar atmosphere in which the temperature gradient is highest.

A

Transition region

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19
Q

Identify the photosphere solar activity feature that is abnormally cold because of strong magnetic field.

20
Q

The Babcock model describes how the solar wind is generated: True or False?

21
Q

Identify the name given to a sudden brightening of electromagnetic waves from the sun.

22
Q

Identify when the average solar wind is faster: solar maximum or solar minimum.

A

Solar minimum

23
Q

The interplanetary magnetic field (IMF) is more azimuthal at Neptune than Earth: True or False?

24
Q

Identify the most likely repetition period for high-speed streams at Earth.

25
Explain what it means to “scope” a space mission. What are the start and end points?
Scoping defines objectives, constraints, and timelines from initial concept to mission end.
26
Define and distinguish coronal holes and coronal streamers. What are their features? Why?
Holes: open field lines, high-speed wind. Streamers: closed loops, slow wind.
27
Identify the two influences that combine to produce the Parker spiral shape of the IMF.
Solar wind outflow and solar rotation.
28
Hand-sketch the internal structure of the sun. What are the regions? What happens in each?
Core (fusion), Radiative Zone, Convective Zone, Photosphere, Chromosphere, Corona.
29
Hand-sketch a diagram showing the relationship between solar granules and spicules.
Granules: convection cells; spicules: jets in chromosphere.
30
Explain the physics and math of why the sun’s corona is not in hydrostatic balance.
Thermal pressure > gravity; use hydrostatic eq: dP/dr = -ρg
31
Charged particles never cross magnetic field lines: True or False?
False
32
Identify the direction of the electric current across the dayside magnetopause.
Dawn to dusk
33
Which radiation belt is produced by cosmic rays: inner or outer?
Inner
34
Identify the primary heat source for the troposphere.
Infrared radiation from Earth
35
Identify the layer of the ionosphere that completely disappears at night.
D layer
36
How long does an isolated auroral substorm typically last: hours, days or weeks?
Hours
37
Identify the dataset the Space Weather Prediction Center uses to classify Solar Radiation Storms.
GOES proton flux
38
Identify the space weather influence most likely to shorten the life of astronauts.
Solar radiation
39
Polar cap absorption is produced by solar flare x-rays: True or False?
True
40
Identify the two quantities that are in perfect balance at the location of the dayside magnetopause.
Magnetic pressure and thermal pressure
41
Identify the three types of alerts issued by the Space Weather Prediction Center.
Solar radiation storm, geomagnetic storm, radio blackout
42
Explain how space weather can adversely affect spacecraft electronics. What is the most likely cause?
Charged particles cause single-event upsets or damage electronics.
43
Hand-sketch the physics of auroral substorms. When do they occur? What happens during each phase?
Growth (tail stretching), expansion (brightening), recovery (calm)
44
Sketch a diagram explaining why the ionosphere is structured in layers. What are the competing influences?
Ionization vs recombination rates by altitude
45
Sketch a diagram of shortwave fadeout. Where and when does it occur? Why? What are its effects?
Occurs on dayside, D-layer overionized by solar flare, causes radio blackout