Sarah Vaughan, Studio Orchestra Golden Hits C'est La Vie Sarah Vaughan, Studio Orchestra Golden Hits MistyĮarl Klugh Solo Guitar It's Only a Paper MoonĬharles Mingus Large Ensemble The Shoes of teh Fisherman's Wife The Shoes of the Fisherman's Wife are Some Jive Ass SlippersĪndy Bey, Peter Washington, Kenny Washington Ain't Necessarily So Someone to Watch Over Me Wes Montgomery, Wynton Kelly, Jimmy Cobb, Paul Chambers Smokin' At the Half Note No Blues Wes Montgomery, Studio Orchestra A Day in the Life Willow Weep For Me The Clayton-Hamilton Jazz Orchestra Live at MCG Lullaby of the Leaves John Coltrane, McCoy Tyner, Jimmy Garrison, Elvin Jones Ballads Say It Over and Over AgainĬlifford Brown, Max Roach, Harold Land, Richie Powell, George Morrow Study in Brown Cherokee McCoy Tyner, Al Foster, George Mraz McCoy Tyner Plays John Coltrane Crescent Toots Thielemans, Michael Lang, Dave Carpenter, Peter Erskine East Coast/West Coast Blue in Green Pat Martino, Joey DeFrancesco, Billy Hart Live at Yoshi's All Blues Wynton Marsalis, Wes Anderson, Wycliffe Gordon, Herlin Riley, Marcus Roberts, Reginald Veal, Todd Williams The Original Soundtrack from Tune in Tomorrow Don't Run From Fun Gary Burton, Steve Swallow, Mike Hyman, Makoto Ozone Real Life Hits Ladies in Mercedes GĬhick Corea, Dave Weckl, John Patitucci Akoustic Band Terminal Baggage ClaimĪnthony Wilson Ensemble Goat Hill Junket Stairway to the Stars Spike Wilner, Plays Monk and Ellington, U. Leon Lee Dorsey, Cantaloupe Island, Sister Sadie Jesse Davis, Live at Smalls Jazz Club, Love For Sale Jazz Defenders, Scheming, Top-Down Tourismīobby Watson, Back Home in Kansas City, Back Home in Kansas CityĮric Alexander, A New Beginning, Blues for Diane (alt take) George Coleman, The Quartet, East Ninth Street Blues Gaetano Letizia, Orange Sunset, Expanding Realityĭavid Larsen, The Peplowski Project, All the Things You AreĪl Cohn – Zoot Sims, Easy as Pie, Blue Hodgeĭerrick Gardner, Pan Africa, Blues for the DiasporaĬanadian Jazz Collective, Septology, Terre de Dusable Gaetano Letizia, Chartreuse, Expanding Reality (2001a,b) developed algorithms for retrieving rain rate (R) as well as Do, Nw and m using βe f f in combination with the measurement pair (Zh, Zdr).Bob Brookmeyer, The Blues Hot and Cold, Hot and Cold BluesĬlark Terry – Bob Brookmeyer, Complete Studio Sessions, Step Right Up The slope of βe f f such that the same relation between Kdp /Nw and Do is preserved on average. Instead it pulls apart when it grows to around 4 millimeters or more. This time, the surface tension loses and the large raindrop ceases to exist. Once the size of a raindrop gets too large, it will eventually break apart in the atmosphere back into smaller drops. The surface tension at the top allows the raindrop to remain more spherical while the bottom gets more flattened out.Įven as a raindrop is falling, it will often collide with other raindrops and increase in size. At the top, small air circulation disturbances create less air pressure.
The reason is due to their speed falling through the atmosphere.Īir flow on the bottom of the water drop is greater than the airflow at the top. Flattened on the bottom and with a curved dome top, raindrops are anything but the classic tear shape. The raindrop becomes more like the top half of a hamburger bun. The reason is the flow of air around the drop.Īs the raindrop falls, it loses that rounded shape. On smaller raindrops, the surface tension is stronger than in larger drops. The cause is the weak hydrogen bonds that occur between water molecules. This surface tension is the "skin" of a body of water that makes the molecules stick together. Raindrops start to form in a roughly spherical structure due to the surface tension of water. High in the atmosphere, water collects on dust and smoke particles in clouds.
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