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SPS 5010 ASTROPHYSICS 1: STELLAR<br />

STRUCTURE AND EVOLUTION (3 credits).<br />

Introduces basic interior structural equations,<br />

energy generation processes, opacity, energy transport,<br />

radiation transport in stellar atmospheres, star<br />

formation, late stages <strong>of</strong> stellar evolution, stellar<br />

binaries and clusters. Special emphasis on analytic<br />

and numerical models relevant to the sun. Prerequisites:<br />

PHY 3060, SPS 1010.<br />

SPS 5011 ASTROPHYSICS 2: GALACTIC<br />

STRUCTURE AND COSMOLOGY (3 credits).<br />

Includes formation and evolution <strong>of</strong> the Galaxy,<br />

including stellar populations and kinematics, spiral<br />

density theory; extragalactic astronomy, active<br />

galactic nuclei, Hubble’s law, large-scale structure;<br />

and cosmology, including inflationary cosmology<br />

and the particle physics connection. Prerequisites:<br />

SPS 5010.<br />

SPS 5020 SPACE PHYSICS 1: THE LOW-<br />

ENERGY UNIVERSE (3 credits). Introduces<br />

low-energy space plasma physics including the<br />

statistical behavior <strong>of</strong> plasmas, kinetic theory and<br />

magnetohydrodynamics. Emphasizes solar system<br />

space plasma physics and the sun-Earth connection<br />

including magnetospheric physics. Prerequisites:<br />

PHY 3440.<br />

SPS 5021 SPACE PHYSICS 2: THE HIGH-<br />

ENERGY UNIVERSE (3 credits). The theoretical<br />

background and methods for observing gamma rays,<br />

x-rays, high energy electrons and heavy particles,<br />

cosmic rays, neutrons and gravitational waves from<br />

both spacecraft and Earth. (Requirement: Prerequisite<br />

course or instructor approval.) Prerequisites:<br />

SPS 4025.<br />

SPS 5030 PLANETARY SCIENCE 1: INTERI-<br />

ORS (3 credits). Mechanical and thermal processes<br />

governing the interior structure and surfaces <strong>of</strong><br />

the major and minor planetary bodies <strong>of</strong> the solar<br />

system. Includes the planetary crust, mantle, core,<br />

core-mantle interface, seismicity, density and elastic<br />

constants. (Requirement: Prerequisite course or<br />

instructor approval.) Prerequisites: SPS 3010.<br />

SPS 5031 PLANETARY SCIENCE 2: ATMO-<br />

SPHERES (3 credits). Principles governing the<br />

evolution, composition and retention <strong>of</strong> planetary<br />

atmospheres and the interplanetary environment.<br />

Includes the neutral atmosphere, photochemical<br />

processes, diffusion dynamics and planetary<br />

ionospheres and magnetospheres. Prerequisites:<br />

SPS 4030.<br />

SPS 5050 ASTRODYNAMICS (3 credits). Includes<br />

the gravitational force, circular restricted threebody<br />

problem, many-bodies problem, perturbation<br />

theory, rocket dynamics, transfer orbits, motion <strong>of</strong><br />

an artificial satellite and interplanetary trajectories.<br />

Prerequisites: SPS 3030.<br />

138 <strong>Florida</strong> Institute <strong>of</strong> Technology<br />

SPS 5088 SPECIAL TOPICS IN SPACE SCI-<br />

ENCES (3 credits). Investigates specific problems<br />

in the space sciences. (Requirement: <strong>Department</strong><br />

head approval.)<br />

SPS 5089 SPECIAL TOPICS IN SPACE SCI-<br />

ENCES (3 credits). Investigates specific problems<br />

in the space sciences. (Requirement: <strong>Department</strong><br />

head approval.) Prerequisites: SPS 5088.<br />

SPS 5090 SPECIAL TOPICS IN OBSERVA-<br />

TIONAL ASTRONOMY 1 (3 credits). Participation<br />

in advanced observing programs at the <strong>university</strong>’s<br />

observatories. (Requirement: <strong>Department</strong> head<br />

approval.)<br />

SPS 5091 SPECIAL TOPICS IN OBSERVA-<br />

TIONAL ASTRONOMY 2 (3 credits). Participation<br />

in advanced observing programs at the <strong>university</strong>’s<br />

observatories. (Requirement: <strong>Department</strong> head<br />

approval.) Prerequisites: SPS 5090.<br />

SPS 5999 THESIS (0-6 credits). Individual work<br />

under the direction <strong>of</strong> a member or members <strong>of</strong> the<br />

graduate faculty on a selected topic in space sciences.<br />

(Requirement: <strong>Department</strong> head approval.)<br />

SPS 6001 INDIVIDUAL STUDIES (1-3 credits).<br />

Preparation for doctoral qualifying examination<br />

by individual studies under faculty supervision.<br />

(Requirement: <strong>Department</strong> head approval.)<br />

SPS 6090 RESEARCH (1-6 credits). Research<br />

leading to the doctoral dissertation. (Requirement:<br />

<strong>Department</strong> head approval.)<br />

SPS 6999 DISSERTATION (0-9 credits). Preparation<br />

<strong>of</strong> doctoral dissertation. (Requirement:<br />

Admission to doctoral candidacy and department<br />

head approval.)<br />

SOFTWARE ENGINEERING<br />

SWE 5001 SOFTWARE ENGINEERING 1 (3<br />

credits). The application <strong>of</strong> engineering rigor to<br />

all phases <strong>of</strong> the s<strong>of</strong>tware development life cycle;<br />

requirements elicitation and analysis, s<strong>of</strong>tware<br />

architecture, s<strong>of</strong>tware design and construction,<br />

s<strong>of</strong>tware integration and test, and s<strong>of</strong>tware maintenance.<br />

Students work individually to develop a<br />

s<strong>of</strong>tware system from an initial problem statement<br />

through release <strong>of</strong> the completed product.<br />

SWE 5002 SOFTWARE ENGINEERING 2 (3<br />

credits). The application <strong>of</strong> engineering rigor and<br />

team coordination to develop a s<strong>of</strong>tware product.<br />

Provided with an initial problem statement, teams<br />

create and document their own disciplined procedures<br />

for each phase <strong>of</strong> the s<strong>of</strong>tware development<br />

life cycle, then develop the s<strong>of</strong>tware according to<br />

their own documented processes and finally provide<br />

in-depth critiques <strong>of</strong> the processes they followed.<br />

Prerequisites: SWE 5001.

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