The Everett Human Services Program: Alumni Attitudes and Perceptions

Summary and analysis of a survey of graduates of the Everett Human Services Program

Prospectus, September 24, 1980

RODNEY DANGERFIELD GETS SOME RESPECT FROM PC; PCF group greets newcomers; Parkland offers COSMOS telecourse; Clerks to be on campus to register voters; Women\u27s Program discusses importance of adequate diet; Breakdown of budget: Where does all your money go?; Women\u27s Program presents last of self-care series; Parkland College Board of Trustees meets; Members needed; A friend is someone who...; Family Life Program offers Living in Step ; Chimera Inc. offers workshop; PACT presents seminar for expectant parents; Steve Goodman: A talented performer; The Ducks have a good time; Rodney Dangerfield: I don\u27t get no respect; He will always get respect in Champaign-Urbana ; Francis named Outstanding Young Men of America ; Eisner to hold celebration; Classifieds; Showcase and workshop Oct. 8; PACT presents program: Early childhood; Volleyballers win two; Upsets spoil Fast Freddy; All you lost freshman-- pay attention to this story; Fast Freddy Contesthttps://spark.parkland.edu/prospectus_1980/1020/thumbnail.jp

Campus Vol V N 1

Rounds, Dave. Cover. Picture. 0.; Rounds, Dave. Untitled. Picture. 2. Olwin, Lynn. homecoming . Prose. 4.; Trimble, John. To Denison . Picture. 6. Cover, Frank. A Remembrance of Things Past. Or, Gee, I\u27d Give the World to See That Ol\u27 Gang of Mine . Prose. 8. Opteker, Pat. New Boy . Prose. 10. Gould, Jim. Untitled. Prose. 11. Rounds, Dave. Untitled. Cartoon. 11. Yearling, Joe. Pigskin greats of Yesteryear . Prose. 14. Gould, Jim. Untitled. Prose. 16. Gould, Jim. Freshman Foto Quiz . Picture. 18. Hawk, Pete. Home Was Never Like This . 20. Pierson, Pete. Homecoming 1950 . cartoon. 12. Pierson, Pete. A View of the Campus . Cartoon. 23

Prospectus, October 1, 1980

HAVE YOU REGISTERED TO VOTE YET? REGISTER THE PAINLESS WAY--ON CAMPUS; Election \u2780: The man behind the woman; Handicrafts taught to senior citizens; Got a pet peeve, gripe, or opinion? Write PROSPECTUS\u27 editor!; MMWW gives calendar of topics; Make Christmas gift decorations now; Student Government will hold O.RG.I.I. in Lounge; Record Enrollment: Fall enrollment sets new record; Activities set for Society; Insurance offered; No overdubbing results in very, very good record; Letters to the editor: Student wants late breakfast; Our Mistake!; Urbana student wins PC faculty wives\u27 $200; Park district has youth fall classes; Give Blood Today; Science You Can See: The chemistry of photography; Parkland student reps needed for committees; New officers named for Parkland\u27s PATH; Children\u27s art exhibit to be Oct. 4, 9-9, Market Place Mall; Arts activities and events need co-sponsors; PLATO proves very popular; Peptic ulcers October 7 topic; PCF to hear Christian teachers; Need it? Financial aid still available; CPA Accounting Careers Conference to be Nov. 15; Classifieds; Football/tennis intermurals begin; Champaign Park District organizes basketball league; PC Datebook; Jeff Dodson places second in LT gold invitational; Women\u27s V-ball record upped; PC baseball player wins; Gal Friday tries predicting; Fast Freddy Contesthttps://spark.parkland.edu/prospectus_1980/1019/thumbnail.jp

Expressions 1988

https://openspace.dmacc.edu/expressions/1031/thumbnail.jp

LSST Science Book, Version 2.0

A survey that can cover the sky in optical bands over wide fields to faint magnitudes with a fast cadence will enable many of the exciting science opportunities of the next decade. The Large Synoptic Survey Telescope (LSST) will have an effective aperture of 6.7 meters and an imaging camera with field of view of 9.6 deg^2, and will be devoted to a ten-year imaging survey over 20,000 deg^2 south of +15 deg. Each pointing will be imaged 2000 times with fifteen second exposures in six broad bands from 0.35 to 1.1 microns, to a total point-source depth of r~27.5. The LSST Science Book describes the basic parameters of the LSST hardware, software, and observing plans. The book discusses educational and outreach opportunities, then goes on to describe a broad range of science that LSST will revolutionize: mapping the inner and outer Solar System, stellar populations in the Milky Way and nearby galaxies, the structure of the Milky Way disk and halo and other objects in the Local Volume, transient and variable objects both at low and high redshift, and the properties of normal and active galaxies at low and high redshift. It then turns to far-field cosmological topics, exploring properties of supernovae to z~1, strong and weak lensing, the large-scale distribution of galaxies and baryon oscillations, and how these different probes may be combined to constrain cosmological models and the physics of dark energy.Comment: 596 pages. Also available at full resolution at http://www.lsst.org/lsst/sciboo

Comparison of Continuous and Filter-Based Carbon Measurements at the Fresno Supersite

Results from six continuous and semicontinuous black carbon (BC) and elemental carbon (EC) measurement methods are compared for ambient samples collected from December 2003 through November 2004 at the Fresno Supersite in California. Instruments included a multi-angle absorption photometer (MAAP; wavelength 670 nm); a dual-wavelength (wavelengths 370 and 880 nm) aethalometer; seven-color (wavelengths 370, 470, 520, 590, 660, 880, and 950 nm) aethalometers; the Sunset Laboratory carbon aerosol analysis field instrument; a photoacoustic light absorption analyzer (wavelength 1047 nm); and the R&P 5400 ambient carbon particulate monitor. All of these acquired BC or EC measurements over periods of 1 min to 1 hr. Twenty-fourhour integrated filter samples were also acquired and analyzed by the Interagency Monitoring of Protected Visual Environments (IMPROVE) thermal/optical reflectance carbon analysis protocol. Site-specific mass absorption efficiencies estimated by comparing light absorption with IMPROVE EC concentrations were 5.5m2/g for the MAAP, 10 m2/g for the aethalometer at a wavelength of 880 nm, and 2.3 m2/g for the photoacoustic analyzer; these differed from the default efficiencies of 6.5, 16.6, and 5m2/g, respectively. Scaling absorption by inverse wavelength did not provide equivalent light absorption coefficients among the instruments for the Fresno aerosol measurements. Ratios of light absorption at 370 nm to those at 880 nm from the aethalometer were nearly twice as high in winter as in summer. This is consistent with wintertime contributions from vehicle exhaust and from residential wood combustion, which is believed to absorb more shorter-wavelength light. To reconcile BC and EC measurements obtained by different methods, a better understanding is needed of the wavelength dependence of light-absorption and mass-absorption efficiencies and how they vary with different aerosol composition