, Maria Consiglio Buonocore1, Domenico Cicala1, Anna Nastro1 and Emilio Cianciulli1
(1)
Division of Pediatric Neuroradiology, Department of Neurosciences, Santobono Pausilipon Children’s Hospital, Naples, Italy
(2)
Department of Neurosciences, Service of Neuroradiology, Santobono Pausilipon Children’s Hospital, Via Mario Fiore n.6, Naples, 80129, Italy
(3)
Division of Radiology, Department of Neurosciences, Federico II University, Via Pansini n. 5, Naples, Italy
26.1 Introduction
Pilocytic astrocytoma (PA) is the most common pediatric cerebellar neoplasm and the most common pediatric glioma, constituting 85 % of all cerebellar astrocytomas and 10 % of all cerebral astrocytomas in this age group [1]. PAs are usually clinically benign and are classified as grade I by the World Health Organization (WHO) [2].
The incidence is approximately 4.8 cases per million people per year, with 2.3–6 % of all brain tumors classified as PA [3]. They have a peak incidence between the age of 5 and 13 years and occur equally frequent in boys and girls [1]. Cerebellar astrocytomas are usually sporadic, but association with neurofibromatosis type 1, Turcot syndrome, PHACE(S) syndrome, and Ollier’s disease has been reported [4]. The prognosis depends particularly on tumor characteristics (location, gross structure, and size) and the completeness of resection. Complete resection, hemispheric location, small size, and presence of cysts are favorable prognostic factors [5].
They are potentially curable by surgery and are associated with a longer survival, with the 25 years survival rate being close to 90 % [6].
Very rarely, a PA may undergo spontaneous malignant transformation and become an anaplastic astrocytoma. Accurate interpretation of imaging studies plays an essential role in directing treatment of these tumors. Patients with cerebellar PA typically present with a gradual onset of symptoms due to the slow growth of the tumor. Common presenting symptoms include headache, nausea and vomiting, and gait imbalance. Common clinical findings include truncal ataxia and papilledema (due to increased intracranial pressure) [7] (Fig. 26.1).
Fig. 26.1
Hydrocephalus (a) coronal TSE T2-image show evident hydrocephalic enlargement of lateral ventricles, area of hyperintensity in periventricular white matter to be attributed to ependymal transudation; (b) sagittal DRIVE T2-image show triventricular hydrocephalus due to obstruction of fourth ventricle by the lesion; (c) sagittal TSE T1 – notice downward tonsillar displacement (arrow) below the McRae line (white line)
26.2 Classifications
26.2.1 Regional
PAs were classified as being located in the cerebellar hemisphere or within the vermis. They were further classified according to the presence of brainstem involvement. It can be difficult to differentiate between tumors that originate primarily within the brainstem and those that originate in the cerebellum when both involve intermediary structures (the middle cerebellar peduncle). The term “transitional astrocytoma” has been applied to PA that has a predominantly cerebellar origin but also involve the brainstem (Fig. 26.2). These tumors show a higher incidence of nonpilocytic histologies and are usually incompletely resectable.
Fig. 26.2
Transitional astrocytoma. Gd-enhanced axial T1-weighted image. Transitional astrocytoma has a predominantly cerebellar origin but also involve the brainstem
This results in a higher proportion of tumor recurrence and, subsequently, a significantly poorer length of survival and long-term neurological outcome than purely cerebellar tumors [8].
26.2.2 Morphologic
The appearance of PA on MR is variable and depends on the tumor’s size and structure. Four predominant imaging patterns of PA have been described:
I.
Typical large cyst with a nonenhancing cyst wall and intensely enhancing mural nodule (sometimes en plaque) (Fig. 26.3)
Fig. 26.3
Pilocytic astrocytoma, type I. (a) Sagital T1 TSE; (b) Axial TSE T1; (c) Coronal T2 TSE; (d) DRIVE T2 Sag; (e) Gd-enhanced Sagittal T1-weighted image. There is a huge cystic lesion with mural nodule. The mural nodule is hypointense on (a, b) T1-weighted images; hyperintense on T2-weighted image (c, d), and enhances markedly (e). The cyst is hypointense on T1-weighted images (a, b), hyperintense on T2-weighted images (c, d). Note nonenhancing cyst wall in (e)
II.
Cystic mass with an enhanced cyst wall and the mural nodule (Figs. 26.4 and 26.5)
Fig. 26.4
Pilocytic astrocytoma, type II. (a), Sagittal DRIVE T2-weighted image; (b, c) Gd-enhanced coronal and axial T1-weighted image. Selected images from an MR of the posterior fossa demonstrates a large cystic mass with peripheral nodular enhancement. It appears to be displaced and compressing the fourth ventricle. Given the patients age, the ventricles appear enlarged in keeping with hydrocephalus
Fig. 26.5
Pilocytic astrocytoma, type II. Gd-enhanced axial T1 fat sat-weighted image. The cystic mass with an enhanced cyst wall and mural nodule
III.
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Tumor appearing largely necrotic with no identifiable mural nodule (falsely cystic) (Fig. 26.6)
Fig. 26.6
Pilocytic astrocytoma type III. (a) Axial FLAIR-weighted image; (b) axial T2-weighted image; (c) Axial T1-weighted image; (d) Gd-enhanced axial T1-weighted image. The tumor appearing largely necrotic with no identifiable mural nodule (falsely cystic)