New Releases by Emily Browning

Whether you''re looking for the right words to send that special person, or the right words to say on Facebook, there''s nothing better than a good romantic poem. This is a collection of some of the best romantic poems, from some of the world''s greatest poets. In just a few words, a romantic poet tells a story that would otherwise require a full length book. Take for example the poem ''Hot and Cold'' by Roald Dahl: A woman who my mother knows Came in and took off all her clothes. Said I, not being very old, ''By golly gosh, you must be cold!'' ''No, no!'' she cried. ''Indeed I''m not! I''m feeling devilishly hot!'' These 38 words generate full length stories within the mind of each reader. A romantic poem touches the heart in a way that mere prose never could. A romantic poem is what you send when you want something priceless for your partner, or potential partner. Within the pages of this book, you''ll find a romantic poem for any occasion, a wedding, a new love, an anniversary, a lost love, or even for a naughty night. Includes poems by: Edwin Arnold W.H. Auden Waitman Barbe Stephen Vincent Benet Francis W. Bourdillon Anne Bradstreet Christopher Brennan Elizabeth Barrett Browning Robert Browning Robert Burns Lord Byron William Cartwright Samuel Taylor Coleridge Emily Dickinson Paul Laurence Dunbar Anne Finch Robert Frost Kahlil Gibran John Keats Walter Savage Landor Richard Lovelace Samuel Lover George Lyttelton Edward Bulwer-Lytton Christopher Marlowe JB O''Reilly Li Po Edgar Allen Poe Adelaide Anne Procter Aleksandr Pushkin Helen Steiner Rice Theodore Roethke Dante Rosetti Lady John Scott William Shakespeare Percy Bysshe Shelley Sir Philip Sidney Charles Swain Kuan Tao-Sheng Alfred, Lord Tennyson Sara Teasdale Walt Whitman Oscar Wilde William Wordsworth William Butler Yeats

The revised age models for the upper Oligocene to middle Miocene interval of the Marion Plateau have been used to identify eleven sequence boundaries and sequences sets at the Marion Plateau; MSA1.2 (23.1 Ma), MSA1.4 (22.1 Ma), MSA2.1 (21.2 Ma), MSB1.1 (18.4 Ma), MSB1.2 (17.3 Ma), MSB2.1 (16.5 Ma), MSB2.2 (15.6 Ma), MSB2.3 (14.8 Ma), MSB3.1 (13.6 Ma), MSB3.2 (12.9 Ma), and MSB3.3 (11.8 Ma). The complementary Miocene oxygen isotope events Mi1, Mi1a, Mi1aa, Mi2, Mi2b, Mi3a, Mi3, Mi4, Mi5a, Mi5, and Mi6 are recognized in the Marion Plateau sequences. In addition correlation to sequences on the New Jersey margin, the Gulf of Papua, Great Australian Bight, and McMurdo Sound Antarctica indicate that these sequences are controlled by glacio-eustasy, primarily the increase of ice volume on Antarctica. Changes in the preservation, assemblage structure and diversity of calcareous nannofossils as well as %planktic foraminifera, %neritics coincide with transgressive phases and sequence boundaries. The principles of ''highstand shedding'' are illustrated at the Marion Plateau by enhanced preservation of calcareous nannofossil, deposition of glauconite, unconformities and condensed intervals associated with early to middle Miocene sequence boundaries. Variations in surface water nutrient and temperature conditions at the Marion Plateau throughout the Miocene coincide with climatic events of the early Miocene (23 - 17 Ma), the Middle Miocene Climatic Optimum (17.6 - 15.4 Ma), and Middle Miocene Climatic Transition (14.8 - 13.8 Ma), and the stepwise growth of ice sheets on Antarctica. Calcareous nannofossil communities show evidence for precessional and eccentricity orbital forcing during the Middle Miocene Climatic Optimum, as well as a significantly cooler surface water mass at the Marion Plateau coinciding with the onset of the Middle Miocene Climatic Transition and Mi3a (14.8 Ma) glacial event. Changes in surface water fertility and temperature during the Middle Miocene Climatic Optimum agree with other studies that posit growth of significant ice volume on Antarctica starting as early as ~17.35 Ma. Further evidence for significant cooling at the Mi3a (14.8 Ma) glacial event agrees with studies suggesting a step-wise cooling for the formation of a semi- permanent Antarctic ice sheet and thermohaline circulation, starting first at 14.8 Ma (Mi3a) and intensifying at 13.9 Ma (Mi3).