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The Acra (also spelled Akra, from Ancient Greek: Ἄκρα, Hebrew: חקרא ,חקרה Ḥaqra(h)), with the meaning of "stronghold" (see under "Etymology"), was a place in Jerusalem thought to have had a fortified compound built by Antiochus Epiphanes, ruler of the Seleucid Empire, following his sack of the city in 168 BCE. The name Acra was also used at a later time for a city quarter probably associated with the by-then destroyed fortress, known in his time to Josephus (1st century CE) as both Acra and "the lower city". The fortress played a significant role in the events surrounding the Maccabean Revolt, which resulted in the formation of the Hasmonean Kingdom. The "upper city" was captured by Judas Maccabeus, with the Seleucid garrison taking refuge in the "Acra" below, and the task of destroying this last enemy stronghold inside Jerusalem fell to Simon Maccabeus surnamed Thassi. Knowledge about the Acra is based almost exclusively on the writings of Josephus, which are of a later date, and on the First and Second Books of Maccabees, which were written not long after the described events. The exact location of Acra within Jerusalem, and even the meaning of the term—fortress, fortified compound inside the city, or compound with an associated fortress—is critical to understanding Hellenistic Jerusalem, but it remains a matter of ongoing discussion. The fact that Josephus has used the name interchangeably with 'the lower city' certainly does not help. Historians and archaeologists have proposed various sites around Jerusalem, relying initially mainly on conclusions drawn from literary evidence. This approach began to change in the light of excavations which commenced in the late 1960s. New discoveries have prompted reassessments of the ancient literary sources, Jerusalem's geography, and previously discovered artifacts. The more recent theories combine archaeological and textual evidence and favour locations near the Temple Mount and south of it, but there are alternative theories as well (see "Location"). The ancient Greek term acra was used to describe other fortified structures during the Hellenistic period. The Acra is often called the Seleucid Acra to distinguish it from references to the Ptolemaic Baris as an acra and from the later city quarter of Jerusalem which inherited the name Acra. (Full article...) |
The Acra (also spelled Akra, from Ancient Greek: Ἄκρα, Hebrew: חקרא ,חקרה Ḥaqra(h)), with the meaning of "stronghold" (see under "Etymology"), was a place in Jerusalem thought to have had a fortified compound built by Antiochus Epiphanes, ruler of the Seleucid Empire, following his sack of the city in 168 BCE. The name Acra was also used at a later time for a city quarter probably associated with the by-then destroyed fortress, known in his time to Josephus (1st century CE) as both Acra and "the lower city". The fortress played a significant role in the events surrounding the Maccabean Revolt, which resulted in the formation of the Hasmonean Kingdom. The "upper city" was captured by Judas Maccabeus, with the Seleucid garrison taking refuge in the "Acra" below, and the task of destroying this last enemy stronghold inside Jerusalem fell to Simon Maccabeus surnamed Thassi. Knowledge about the Acra is based almost exclusively on the writings of Josephus, which are of a later date, and on the First and Second Books of Maccabees, which were written not long after the described events. The exact location of Acra within Jerusalem, and even the meaning of the term—fortress, fortified compound inside the city, or compound with an associated fortress—is critical to understanding Hellenistic Jerusalem, but it remains a matter of ongoing discussion. The fact that Josephus has used the name interchangeably with 'the lower city' certainly does not help. Historians and archaeologists have proposed various sites around Jerusalem, relying initially mainly on conclusions drawn from literary evidence. This approach began to change in the light of excavations which commenced in the late 1960s. New discoveries have prompted reassessments of the ancient literary sources, Jerusalem's geography, and previously discovered artifacts. The more recent theories combine archaeological and textual evidence and favour locations near the Temple Mount and south of it, but there are alternative theories as well (see "Location"). The ancient Greek term acra was used to describe other fortified structures during the Hellenistic period. The Acra is often called the Seleucid Acra to distinguish it from references to the Ptolemaic Baris as an acra and from the later city quarter of Jerusalem which inherited the name Acra. (Full article...) |
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Combe Hill is a causewayed enclosure, near Eastbourne in East Sussex, on the northern edge of the South Downs. It consists of an inner circuit of ditches and banks, incomplete where it meets a steep slope on its north side, and the remains of an outer circuit. Causewayed enclosures were built in England from shortly before 3700 BC until at least 3500 BC; they are characterized by the full or partial enclosure of an area with ditches that are interrupted by gaps, or causeways. Their purpose is not known; they may have been settlements, meeting places, or ritual sites. The historian Hadrian Allcroft included the site in his 1908 book Earthwork of England, and in 1930 E. Cecil Curwen listed it as a possible Neolithic site in a paper which attempted to provide the first list of all the causewayed enclosures in England. The enclosure has been excavated twice: in 1949, by Reginald Musson, and in 1962, by Veronica Seton-Williams, who used it as a training opportunity for volunteers. Charcoal fragments from Musson's dig were later dated to between 3500 and 3300 BC. Musson also found a large quantity of Ebbsfleet ware pottery in one of the ditches. Seton-Williams found three polished stone axes deposited in another ditch, perhaps not long after it had been dug. The site is only 800 m (870 yd) from Butts Brow, another Neolithic enclosure, and the two locations are visible from each other; both sites may have seen Neolithic activity at the same time. (Full article...) |
Combe Hill is a causewayed enclosure, near Eastbourne in East Sussex, on the northern edge of the South Downs. It consists of an inner circuit of ditches and banks, incomplete where it meets a steep slope on its north side, and the remains of an outer circuit. Causewayed enclosures were built in England from shortly before 3700 BC until at least 3500 BC; they are characterized by the full or partial enclosure of an area with ditches that are interrupted by gaps, or causeways. Their purpose is not known; they may have been settlements, meeting places, or ritual sites. The historian Hadrian Allcroft included the site in his 1908 book Earthwork of England, and in 1930 E. Cecil Curwen listed it as a possible Neolithic site in a paper which attempted to provide the first list of all the causewayed enclosures in England. The enclosure has been excavated twice: in 1949, by Reginald Musson, and in 1962, by Veronica Seton-Williams, who used it as a training opportunity for volunteers. Charcoal fragments from Musson's dig were later dated to between 3500 and 3300 BC. Musson also found a large quantity of Ebbsfleet ware pottery in one of the ditches. Seton-Williams found three polished stone axes deposited in another ditch, perhaps not long after it had been dug. The site is only 800 m (870 yd) from Butts Brow, another Neolithic enclosure, and the two locations are visible from each other; both sites may have seen Neolithic activity at the same time. (Full article...) |
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The Temple of Eshmun (Arabic: معبد أشمون) is an ancient place of worship dedicated to Eshmun, the Phoenician god of healing. It is located near the Awali river, 2 kilometres (1.2 mi) northeast of Sidon in southwestern Lebanon. The site was occupied from the 7th century BC to the 8th century AD, suggesting an integrated relationship with the nearby city of Sidon. Although originally constructed by Sidonian king Eshmunazar II in the Achaemenid era (c. 529–333 BC) to celebrate the city's recovered wealth and stature, the temple complex was greatly expanded by Bodashtart, Yatonmilk and later monarchs. Because the continued expansion spanned many centuries of alternating independence and foreign hegemony, the sanctuary features a wealth of different architectural and decorative styles and influences. The sanctuary consists of an esplanade and a grand court limited by a huge limestone terrace wall that supports a monumental podium which was once topped by Eshmun's Greco-Persian style marble temple. The sanctuary features a series of ritual ablution basins fed by canals channeling water from the Asclepius river (modern Awali) and from the sacred "YDLL" spring; these installations were used for therapeutic and purificatory purposes that characterize the cult of Eshmun. The sanctuary site has yielded many artifacts of value, especially those inscribed with Phoenician texts, such as the Bodashtart inscriptions and the Eshmun inscription, providing valuable insight into the site's history and that of ancient Sidon. The Eshmun Temple was improved during the early Roman Empire with a colonnade street, but declined after earthquakes and fell into oblivion as Christianity replaced polytheism and its large limestone blocks were used to build later structures. The temple site was rediscovered in 1900 by local treasure hunters who stirred the curiosity of international scholars. Maurice Dunand, a French archaeologist, thoroughly excavated the site from 1963 until the beginning of the Lebanese Civil War in 1975. After the end of the hostilities and the retreat of Israel from Southern Lebanon, the site was rehabilitated and inscribed to the World Heritage Site tentative list. (Full article...) |
The Temple of Eshmun (Arabic: معبد أشمون) is an ancient place of worship dedicated to Eshmun, the Phoenician god of healing. It is located near the Awali river, 2 kilometres (1.2 mi) northeast of Sidon in southwestern Lebanon. The site was occupied from the 7th century BC to the 8th century AD, suggesting an integrated relationship with the nearby city of Sidon. Although originally constructed by Sidonian king Eshmunazar II in the Achaemenid era (c. 529–333 BC) to celebrate the city's recovered wealth and stature, the temple complex was greatly expanded by Bodashtart, Yatonmilk and later monarchs. Because the continued expansion spanned many centuries of alternating independence and foreign hegemony, the sanctuary features a wealth of different architectural and decorative styles and influences. The sanctuary consists of an esplanade and a grand court limited by a huge limestone terrace wall that supports a monumental podium which was once topped by Eshmun's Greco-Persian style marble temple. The sanctuary features a series of ritual ablution basins fed by canals channeling water from the Asclepius river (modern Awali) and from the sacred "YDLL" spring; these installations were used for therapeutic and purificatory purposes that characterize the cult of Eshmun. The sanctuary site has yielded many artifacts of value, especially those inscribed with Phoenician texts, such as the Bodashtart inscriptions and the Eshmun inscription, providing valuable insight into the site's history and that of ancient Sidon. The Eshmun Temple was improved during the early Roman Empire with a colonnade street, but declined after earthquakes and fell into oblivion as Christianity replaced polytheism and its large limestone blocks were used to build later structures. The temple site was rediscovered in 1900 by local treasure hunters who stirred the curiosity of international scholars. Maurice Dunand, a French archaeologist, thoroughly excavated the site from 1963 until the beginning of the Lebanese Civil War in 1975. After the end of the hostilities and the retreat of Israel from Southern Lebanon, the site was rehabilitated and inscribed to the World Heritage Site tentative list. (Full article...) |
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Under the Köppen–Geiger classification, Sydney has a humid subtropical climate (Cfa) with "warm, sometimes hot" summers and "generally mild", to "cool" winters. The El Niño–Southern Oscillation, the Indian Ocean Dipole and the Southern Annular Mode play an important role in determining Sydney's weather patterns: drought and bushfire on the one hand, and storms and flooding on the other, associated with the opposite phases of the oscillation in Australia. The weather is moderated by proximity to the ocean, and more extreme temperatures are recorded in the inland western suburbs because Sydney CBD is more affected by the oceanic climate drivers than the western suburbs. At Sydney's primary weather station at Observatory Hill, extreme temperatures have ranged from 45.8 °C (114.4 °F) on 18 January 2013 to 2.1 °C (35.8 °F) on 22 June 1932. An average of 14.9 days a year have temperatures at or above 30 °C (86 °F) in the central business district (CBD). In contrast, the metropolitan area averages between 35 and 65 days, depending on the suburb. The hottest day in the metropolitan area occurred in Penrith on 4 January 2020, where a high of 48.9 °C (120.0 °F) was recorded. The average annual temperature of the sea ranges from 18.5 °C (65.3 °F) in September to 23.7 °C (74.7 °F) in February. Sydney has an average of 7.2 hours of sunshine per day and 109.5 clear days annually. Due to the inland location, frost is recorded early in the morning in Western Sydney a few times in winter. Autumn and spring are the transitional seasons, with spring showing a larger temperature variation than autumn. Sydney experiences an urban heat island effect. This makes certain parts of the city more vulnerable to extreme heat, including coastal suburbs. In late spring and summer, temperatures over 35 °C (95 °F) are not uncommon, though hot, dry conditions are usually ended by a southerly buster, a powerful southerly that brings gale winds and a rapid fall in temperature. Since Sydney is downwind of the Great Dividing Range, it occasionally experiences dry, westerly foehn winds typically in winter and early spring (which are the reason for its warm maximum temperatures). Westerly winds are intense when the Roaring Forties (or the Southern Annular Mode) shift towards southeastern Australia, where they may damage homes and affect flights, in addition to making the temperature seem colder than it actually is. Rainfall has a moderate to low variability and has historically been fairly uniform throughout the year, although in recent years it has been more summer-dominant and erratic. Precipitation is usually higher in summer through to autumn, and lower in late winter to early spring. In late autumn and winter, east coast lows may bring large amounts of rainfall, especially in the CBD. In the warm season black nor'easters are usually the cause of heavy rain events, though other forms of low-pressure areas, including remnants of ex-cyclones, may also bring heavy deluge and afternoon thunderstorms. 'Snow' was last alleged in 1836, more than likely a fall of graupel, or soft hail; and in July 2008 the Upper North Shore saw a fall of graupel that was mistaken by many for 'snow'. In 2009, dry conditions brought a severe dust storm towards the city.
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Adelaide has a hot-summer Mediterranean climate (Csa) under the Köppen climate classification. The city has hot, dry summers and cool winters with moderate rainfall. Most precipitation falls in the winter months, leading to the suggestion that the climate be classified as a "cold monsoon". Rainfall is unreliable, light and infrequent throughout summer, although heavy falls can occur. The winter has fairly reliable rainfall with June being the wettest month of the year, averaging around 80 mm. Frosts are occasional, with the most notable occurrences in 1908 and 1982. Hail is common in winter. Adelaide is a windy city with significant wind chill in winter, which makes the temperature seem colder than it actually is. Snowfall in the metropolitan area is extremely rare, although light and sporadic falls in the nearby hills and at Mount Lofty occur during winter. Dewpoints in the summer typically range from 8 to 10 °C (46 to 50 °F). There are usually several days in summer where the temperature reaches 40.0 °C (104.0 °F) or above; the frequency of these temperatures has been increasing in recent years. Temperature extremes range from −0.4 °C (31.4 °F), 8 June 1982 to 47.7 °C (117.9 °F), 24 January 2019. The city features 90.6 clear days annually. The average sea temperature ranges from 13.7 °C (56.7 °F) in August to 21.2 °C (70.2 °F) in February. (Full article...) | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
References
[edit]This section contains references and notes. It should be empty.
- ^ "Sydney (Observatory Hill) Period 1991-2020". Bureau of Meteorology. Retrieved 14 April 2020.
- ^ "Sydney (Observatory Hill): all years". Bureau of Meteorology. Retrieved 4 June 2018.
- ^ "Sydney (Observatory Hill): highest temperatures". Bureau of Meteorology. Archived from the original on Sep 27, 2023. Retrieved 23 September 2023.
- ^ "Sydney (Observatory Hill): lowest temperatures". Bureau of Meteorology. Retrieved 23 September 2023.
- ^ "Climate statistics for Australian locations Sydney Airport AMO". Bureau of Meteorology.